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Segmentation of Stochastic Images using ... - Jacobs University

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Chapter 4 Discretization <strong>of</strong> SPDEs<br />

4.3.1 Discretization <strong>of</strong> the Spaces V and S<br />

We approximate the deterministic space V <strong>using</strong> the classical finite element approach. That means<br />

every u ∈ V ⊗ S is approximated by<br />

u(x,ω) ≈ ∑ n i=1 u i(ω)P i (x) , (4.12)<br />

where u i ∈ S and {P i } i=1,...,n is a basis <strong>of</strong> a finite dimensional subspace V h ⊂ V . We identify the<br />

space V h with IR n , because we have to store the coefficients for the basis elements only.<br />

We approximate the stochastic space S in two steps. First, we choose a finite set <strong>of</strong> random<br />

variables ζ =(ζ 1 ,...,ζ m ), span(ζ 1 ,...,ζ m )=S m ⊂S with finite variance and approximate u i ∈ S by<br />

u i (ω) ≈ ∑ m k=1 uk i ζ k (ω) , (4.13)<br />

where the coefficients u k i are deterministic coefficients for the random variables ζ k . Numerical calculations<br />

cannot use the space S m . Hence, we approximate the space S m by <strong>using</strong> the generalized<br />

polynomial chaos [160], cf. Section 3.3. We approximate the random variables ζ i with unknown<br />

distribution in the polynomial chaos by the same number <strong>of</strong> random variables and a prescribed polynomial<br />

degree p:<br />

u ∈ S m,p ⊂ S p : u = ∑ N i=1 u iΨ i (ξ ) . (4.14)<br />

The dimension <strong>of</strong> the space S m,p is N = ( )<br />

m+p<br />

m .<br />

For the finite dimensional subspace IR n ⊗ S p , the problem (4.9) is rewritten as<br />

E(v T Au) = E(v T b) ∀v ∈ IR n ⊗ S p , (4.15)<br />

where A ∈ Sp<br />

n×n is a stochastic matrix.<br />

Using the polynomial chaos basis, i.e. the space S m,p for the stochastic space and V h for the<br />

deterministic space we end up with a huge deterministic equation system to approximate the solution<br />

<strong>of</strong> ∇ · (a∇u) = f given by<br />

∑ N α=1<br />

where the matrices M α,β and L α,β are<br />

(M α,β ) i, j = E (Ψ α Ψ β ) ∫<br />

(<br />

L α,β ) i, j = ∑<br />

k<br />

(<br />

L α,β ) U α = ∑ N α=1 Mα,β F α , (4.16)<br />

(<br />

∑E<br />

γ<br />

D<br />

P i P j dx<br />

Ψ α Ψ β Ψ γ) a k γ<br />

∫<br />

D<br />

∇P i · ∇P j P k dx .<br />

(4.17)<br />

In (4.16) we used the notation F α = ( f i α) for the polynomial chaos representation <strong>of</strong> the quantities.<br />

4.4 Generalized Spectral Decomposition<br />

Selecting suitable subspaces <strong>of</strong> S m,p ⊗IR n and a special basis, which captures the dominant stochastic<br />

effects, we achieve a significant speed-up <strong>of</strong> the solution process and an enormous reduction <strong>of</strong><br />

the memory requirements. In the generalized spectral decomposition (GSD) [113], we approximate<br />

the solution u ∈ L 2 (Ω) ⊗ H 1 (D) by<br />

u(x,ξ ) ≈ ∑ K j=1 λ j(ξ )V j (x) , (4.18)<br />

where V j is a deterministic function, λ j a stochastic function and K the number <strong>of</strong> modes <strong>of</strong> the<br />

decomposition. Thus, the GSD computes a solution where the deterministic and the stochastic basis<br />

40

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