Segmentation of Stochastic Images using ... - Jacobs University
Segmentation of Stochastic Images using ... - Jacobs University
Segmentation of Stochastic Images using ... - Jacobs University
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Chapter 3 SPDEs and Polynomial Chaos Expansions<br />
Definition The n-th central moment <strong>of</strong> a random variable X is<br />
M n (X) = E((X − E(X)) n ) . (3.2)<br />
A famous member <strong>of</strong> this class <strong>of</strong> moments is the second central moment, the variance:<br />
Var(X) = E ( (X − E(X)) 2) . (3.3)<br />
Later we have to evaluate the relation between random variables. A famous tool for this is the<br />
covariance.<br />
Definition The covariance <strong>of</strong> two random variables f ,g with finite second order moments is<br />
Cov( f ,g) = E( f g) − E( f )E(g) . (3.4)<br />
In what follows, it will be necessary to have a set <strong>of</strong> random variables indexed by a spatial position.<br />
This motivates the following definition:<br />
Definition A random field X is a collection <strong>of</strong> random variables indexed by a spatial position x ∈ IR n :<br />
X = {X x |x ∈ IR n } . (3.5)<br />
Random fields are elements <strong>of</strong> a tensor product space consisting <strong>of</strong> functions defined on the Cartesian<br />
product Ω × D. A random field is a function taking two arguments, a random event and a spatial<br />
position. We restrict the investigations to random fields satisfying smoothness assumptions.<br />
Definition Let D ⊂ IR n be the spatial domain <strong>of</strong> the random field and Ω the sample space. The<br />
tensor space L 2 (Ω) ⊗ H 1 (D) is the space <strong>of</strong> random fields satisfying u(ω,·) ∈ H 1 (D) almost sure<br />
and u(·,x) ∈ L 2 (Ω), where H 1 (D) is the usual Sobolev space and<br />
{<br />
∫<br />
}<br />
L 2 (Ω) = f : Ω → IR : f (ω) 2 dω < ∞ . (3.6)<br />
Ω<br />
This is a strong limitation which is typically not satisfied for random fields arising in financial problems<br />
[69, 108]. For image processing problems, this space is reasonable, because H 1 -regularity is<br />
typically assumed for classical image processing tasks [17] and L 2 -regularity <strong>of</strong> the stochastic part<br />
seems reasonable due to the limited energy an image acquisition device detects. Furthermore, the<br />
restriction to random fields with finite variance, i.e. satisfying (3.6), allows a discretization <strong>of</strong> the<br />
random fields <strong>using</strong> polynomial chaos expansions. Random fields will play a crucial role in the presentation<br />
<strong>of</strong> SPDEs, because the locally varying random coefficients <strong>of</strong> the SPDEs are random fields.<br />
3.2 <strong>Stochastic</strong> Partial Differential Equations<br />
We introduce SPDEs following [18] and use an elliptic model equation. The deterministic equation is<br />
−∇ · (a∇u) = f<br />
on D<br />
u = g on ∂D ,<br />
(3.7)<br />
where a is a diffusion coefficient, f a source term, g the boundary condition, and D the deterministic<br />
domain this equation holds in. In this equation, we assumed that we perfectly know the diffusion<br />
coefficient a and the right hand side f . In many applications, these quantities are not known exactly,<br />
but a description <strong>of</strong> the quantities through random fields is possible (see e.g. [8]). Let D be a bounded<br />
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