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Adaptivity with moving grids

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12 C. J. Budd, W. Huang and R. D. Russell<br />

so that<br />

Ω C =[0, 1] n .<br />

To describe a computational mesh in the case of such simply connected<br />

domains we typically divide Ω C ⊂ R n into N n uniform, regular tetrahedra or<br />

cuboids of side proportional to 1/N and volume proportional to 1/N n ,and<br />

we will initially assume that this is the case. In the r-adaptive procedure<br />

considered in this section we consider the mesh points to be joined in a<br />

simple (logically rectangular or triangular) network, the topology of which<br />

(and consequently the ordering of the nodes in the network) is fixed for most<br />

(if not all) of the time during the computation. Indeed, it is this constancy<br />

of ordering which makes the r-adaptive procedure very attractive for finite<br />

element and related computations.<br />

To derive a <strong>moving</strong> mesh, the computational domain <strong>with</strong> its associated<br />

mesh is then mapped to a physical domain Ω P ∈ R n , in which the underlying<br />

PDE is posed. We assume that there is an invertible, adaptive mesh<br />

generating function<br />

F :Ω C → Ω P<br />

describing this map, so that F is smooth on the interior of Ω C and continuous<br />

on Ω C . Throughout this article we will denote variables in Ω C by Greek<br />

letters, e.g., ξ, andinΩ P by Roman letters, x, and consider the function<br />

F(ξ,t)tobetime-dependent. The action of the function F on the fixed<br />

mesh τ C generates a <strong>moving</strong> mesh τ P in the physical domain. An example<br />

of such a mesh is given in Figure 2.1, in which a uniform rectangular mesh<br />

in Ω C is mapped to a mesh τ P . (This map was constructed by using the<br />

optimal transport method described in Section 3.)<br />

In the case where τ C is a uniform rectangular mesh, the resulting mesh<br />

τ P in the physical space is then (in the representative example of a twodimensional<br />

system) given by the points (X i,j ,Y i,j ), where F =(x, y) and<br />

( i<br />

X i,j = x<br />

N , j ) ( i<br />

, Y i,j = y<br />

N N , j )<br />

. (2.1)<br />

N<br />

We assume further that the boundary of ∂Ω C of Ω C is mapped by F to<br />

the boundary of ∂Ω P of Ω P . In some r-adaptive strategies (such as the<br />

multi-equidistribution and/or variational strategies described in Huang and<br />

Russell (1999), the map F is augmented <strong>with</strong> a second map,<br />

∂F : ∂Ω C → Ω P ,<br />

which explicitly describes the map from one boundary to another. This<br />

has the advantage of close control of the meshing strategy right up to the<br />

boundary, but has the disadvantage of introducing extra complexity into<br />

the system. In other algorithms, such as the optimal mapping strategy<br />

(Delzanno, Chacón, Finn, Chung and Lapenta 2008, Budd and Williams

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