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tel-00656013, version 1 - 3 Jan 2012<br />

52 A dynamic multilayer shallow water mo<strong>de</strong>l<br />

It is therefore sufficient to apply Taylor expansions in the vertical direction. Namely,<br />

assuming the velocities are smooth enough, we have the following approximations: for all<br />

1 i N −1, for all z ∈ [z i−1/2,z i+1/2]:<br />

⎧<br />

⎪⎨<br />

⎪⎩<br />

u(z) = ui +O h ,<br />

<br />

u(zi+1/2) = ui+1/2 +O h 2<br />

,<br />

∂zu(z i+1/2) = 2 ui+1 −ui<br />

hi +hi+1<br />

zi+1/2<br />

z i−1/2<br />

zi+1/2<br />

z i−1/2<br />

<br />

+O h 2<br />

,<br />

<br />

u⊗udz = hiui ⊗ui +O h 2<br />

,<br />

<br />

∇xudz = hi∇xui +O h 2<br />

.<br />

(2.2.5)<br />

Next, by the use of the boundary conditions at the bottom (2.1.3) and the or<strong>de</strong>r of magnitu<strong>de</strong><br />

of the variations of the bathym<strong>et</strong>ry (2.2.3), the <strong>de</strong>finition of the approximate reconstructions<br />

of the vertical velocity at the interfaces b<strong>et</strong>ween layers (2.1.7) yields, for all<br />

0 ≤ i ≤ N −1:<br />

<br />

wi+1/2 = w(zi+1/2)+O h 2<br />

.<br />

L<strong>et</strong> us look at the viscous terms with the previous approximations:<br />

∇x ·<br />

zi+1/2<br />

z i−1/2<br />

∇xudz<br />

<br />

=<br />

⎧<br />

⎪⎨<br />

⎪⎩<br />

h1∆xu1 −∇xub ·∇xzb +O(h 2 ) if i = 1,<br />

hi∆xui +O(h 2 ) if i = 2,...,N −1,<br />

∇x ·(hN ∇xuN)+O(h 2 ) if i = N .<br />

Hence, in the equation (2.2.4) for the lowest layer, the non zero boundary terms of the<br />

viscous part cancel each other and we g<strong>et</strong>, using the boundary conditions at the bottom:<br />

∂t(h1u1)+∇x ·(h1u1 ⊗u1)+gh1∇xhN = −gh1∇xzb −w 3/2u 3/2 −κu1 −f (h1u1) ⊥<br />

+µh1∆xu1 +2µ u2 −u1<br />

h1 +h2<br />

<br />

+O h 2<br />

.<br />

For the insi<strong>de</strong> layers, we use again the approximations (2.2.5): the result is obtained easily<br />

because the intermediate layer heights are constant in time and space. Finally, there is<br />

another term in equation (2.2.4) for the highest layer, coming from the time <strong>de</strong>pen<strong>de</strong>ncy<br />

of the highest layer. It is simplified thanks to the boundary conditions at the free surface

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