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Numerical simulation of particle concentration in a turbulent pipe flow Hans Kuerten Maurice Veenman Joost de Hoogh
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Contents DNS - model Concentration equations Space and time discretisation Early results Finite volume method Future planning
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DNS model Direct Numerical Simulation by M. Veenman Axial and tangential direction –Spectral solver Radial direction –Chebychev polynomial expansion Implementation of the concentration equations as a passive scalar
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Concentration equation Boundary conditions Axial and tangential direction: periodic conditions Radial direction:
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Adams-Bashforth time integration
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Simple testing 1. 2. 3. 4.
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First results Movie clip!
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Negative concentration
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Finite volume method Roe’s first order upwind scheme Muscl method (by van Leer) Second/third order depending on parameters r φ z
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Results Muscl method MovieMovie clip!clip!
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Different grid New uniform grid –Radial direction: uniform grid –Tangential direction (MUSCL): half the points Velocity Interpolation
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Mean radius Muscl Fourier 1 st order upwind
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Things still to do Implement diffusion Compare the model with Brethouwer’s results Look into forces acting on the concentration (e.g. gravity)
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