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RANDOM FIELDS AND THEIR GEOMETRY

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22 1. Random fields<br />

Since indicator functions are in K, we can define a process W on RN by<br />

setting<br />

W (λ) = Θ −1 � �<br />

(1.4.22)<br />

� (−∞,λ] ,<br />

where (−∞, λ] = �N j=1 (−∞, λj]. Working through the isomorphisms shows<br />

that W is a complex ν-noise and that �<br />

RN exp(i〈t, λ〉) W (dλ) is (L2 (P) indistinguishable<br />

from) ft. ✷<br />

There is also an inverse 22 to (1.4.19), expressing W as an integral involving<br />

f, but we shall have no need of it and so now turn to some consequences<br />

of Theorems 1.4.3 and 1.4.4.<br />

When the basic field f is real, it is natural to expect a ‘real’ spectral<br />

representation, and this is in fact the case, although notationally it is still<br />

generally more convenient to use the complex formulation. Note firstly that<br />

if f is real, then the covariance function is a symmetric function (C(t) =<br />

C(−t)) and so it follows from the spectral distribution theorem (cf. (1.4.16))<br />

that the spectral measure ν must also be symmetric. Introduce three 23 new<br />

measures, on R+ × R N−1 , by<br />

ν1(A) = ν(A ∩ {λ ∈ R N : λ1 > 0})<br />

ν2(A) = ν(A ∩ {λ ∈ R N : λ1 = 0})<br />

µ(A) = 2ν1(A) + ν2(A)<br />

We can now rewrite24 (1.4.16) in real form, as<br />

�<br />

(1.4.23) C(t) =<br />

cos(〈λ, t〉) µ(dλ).<br />

R+×R N−1<br />

There is also a corresponding real form of the spectral representation<br />

(1.4.19). The fact that the spectral representation yields a real valued processes<br />

also implies certain symmetries 25 on the spectral process W . In particular,<br />

it turns out that there are two independent real valued µ-noises,<br />

22 Formally, the inverse relationship is based on (1.4.22), but it behaves like regular<br />

Fourier inversion. For example, if ∆(λ, η) is a rectangle in R N which has a boundary of<br />

zero ν measure, then<br />

W (∆(λ, η)) = lim<br />

K→∞ (2π)−N<br />

Z K Z K<br />

. . .<br />

−K −K<br />

NY e<br />

k=1<br />

−iλktk − e−iηktk f(t) dt.<br />

−itk<br />

As is usual, if ν(∆(λ, η)) �= 0, then additional boundary terms need to be added.<br />

23Note that if ν is absolutely continuous with respect to Lebesgue measure (so that<br />

there is a spectral density) one of these, ν2, will be identically zero.<br />

24There is nothing special about the half-space λ1 ≥ 0 taken in this representation.<br />

Any half space will do.<br />

25To rigorously establish this we really need the inverse to (1.4.19), expressing W as<br />

an integral involving f, which we do not have.

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