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Solving the Taylor problem with horizontal viscosity
Pieter C. Roos Water Engineering & Management, University of Twente Henk M. Schuttelaars Delft Institutie of Applied Mathematics, TU Delft NCK days 2008, Deltares, Delft, March 2008
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Contents Motivation and goal Background: inviscid Taylor problem
Viscous Taylor problem Results Open channel modes Viscous Taylor solution Conclusions Outlook
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1. Motivation and goal Understand morphodynamics of tidal basins
Tool: process-based model for tidal flow Smooth flow field required add horizontal viscosity Arbitrary box-type geometries Taylor problem
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2. Background: inviscid Taylor problem
Co-tidal and co-range chart Semi-infinite rectangular basin of uniform depth No-normal flow BC Inviscid shallow water eqs. Incoming Kelvin wave Tidal current ellipses Source: Taylor (1921)
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2. Background: inviscid Taylor problem
Co-tidal and co-range chart Semi-infinite rectangular basin of uniform depth Solution as superposition of ‘open channel modes’ Kelvin & Poincaré waves Collocation method Amphidromic system and tidal current ellipses Tidal current ellipses Source: Taylor (1921)
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2. Extending inviscid Taylor problem…
Semi-infinite rectangular basin of uniform depth Solution as superposition of ‘open channel modes’ Extension to arbitrary box-type geometries Problems for flow field at reflex angle-corners Remedy: add viscosity ζ(x,y,t) |u|(x,y) Tidal current ellipses
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3. Viscous Taylor problem
Geometry and boundary conditions Free surface elevation ζ, depth-averaged flow (u,v) No slip at closed boundaries: (u,v)=0 Incoming Kelvin wave from x=+∞ y↑ Kelvin wave B Uniform depth H x=0 x→
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3. Viscous Taylor problem
Geometry and boundary conditions Linearized shallow water equations – at O(Fr0) gζx + ut – fv = ν[uxx+uyy] gζy + vt + fu = ν[vxx+vyy] ζt + [Hu]x + [Hv]y = 0 Acceleration of gravity g, Coriolis parameter f, water depth H, horizontal viscosity ν
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3. Viscous Taylor problem
Geometry and boundary conditions Linearized shallow water equations – at O(Fr0) Solution method Find viscous ‘open channel modes’ Write solution as a superposition of these modes Use collocation method to satisfy no slip BC at x=0
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4. Results: open channel modes
General form: ζ(x,y,t) = Z(y)exp(i[ωt-kx]) + c.c. Angular frequency ω, (complex) wave number k Transverse structure: Z(y) = Z1e-αy + Z2e-βy + Z3eα[y-B] + Z4eβ[y-B] Solvability condition from BCs at y=0,B k, α, β, Zj y↑ B Uniform depth H x=0 x→
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4. Open channel modes inviscid
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4. Open channel modes inviscid viscous
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4. Open channel modes Viscous Kelvin and Poincaré modes
Boundary layers at y=0,B Interior structure similar to inviscid case Viscous dissipation, slight decrease in length scales y↑ B Uniform depth H x=0 x→
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4. Viscous Kelvin mode viscous ζ(x,y,t) u(x,y,t) v(x,y,t)
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4. Viscous Poincaré modes
ζ(x,y,t) u(x,y,t) v(x,y,t)
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4. Viscous Poincaré modes
ζ(x,y,t) u(x,y,t) v(x,y,t)
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4. New modes viscous ζ(x,y,t) u(x,y,t) v(x,y,t)
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4. Viscous Taylor solution
Truncated superposition of open channel modes Incoming Kelvin wave and 2N+1 reflected modes Use collocation method to satisfy no-slip BC at x=0 N+1 points where u=0 and N points where v=0 y↑ u=0 v=0 Kelvin wave x=0 x→
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4. Viscous Taylor solution
ζ(x,y,t) u(x,y,t) v(x,y,t)
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5. Conclusions Taylor problem has been extended to account for horizontally viscous effects No-slip condition at closed boundaries Solution involves viscous open channel modes Viscous Kelvin and Poincaré modes A new type of mode arises, responsible for the transverse boundary layer at x=0
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6. Outlook Details of collocation method
Residual flow and higher harmonics Nonlinear M2-interactions at O(Fr1) M0, M4 Geometrical extension of viscous model To arbitrary box-type geometries smooth flow field Applications: artificial islands, inlets, obstructions
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