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Application and Optimisation of the Spatial Phase Shifting ...

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34 Statistical Properties <strong>of</strong> Speckle Patterns<br />

function, which demonstrates that <strong>the</strong> speckle shape is closely related to <strong>the</strong> aperture´s point spread<br />

function. It assumes its first zero at<br />

∆x<br />

λ z<br />

+ ∆y<br />

≅ 122 . =<br />

D<br />

2 2<br />

d s<br />

,<br />

(2.43)<br />

which gives <strong>the</strong> mean speckle size. The shape <strong>of</strong> R I (∆x, ∆y) is given in Fig. 2.20. If we write <strong>the</strong> intensity<br />

correlation as R I (x 1 , y 1 , x 2 , y 2 )=I(x 1 ,y 1 ) I(x 2 ,y 2 ), we can use <strong>the</strong> independence <strong>of</strong> P 1 <strong>and</strong> P 2 at µ A = 0 to<br />

decompose it into I(x 1 ,y 1 ) I(x 2 ,y 2 )=I 2 , while for µ A = 1 we have P 1 =P 2 <strong>and</strong> obtain I(x 1 ,y 1 )<br />

I(x 1 ,y 1 )=2I 2 =I 2 . The "bias correlation" reflects <strong>the</strong> fact that <strong>the</strong> intensity is never negative, in<br />

contrast to <strong>the</strong> phase <strong>and</strong> its autocorrelation.<br />

2<br />

R I (∆x ,∆y )/ I ¡ 2 ( ) ( )<br />

1.5<br />

1<br />

-3 -2 -1 0 1 2 3<br />

∆<br />

2 2 D<br />

x + ∆y<br />

λ z<br />

Fig. 2.20: Speckle intensity autocorrelation function for a circular scattering spot with uniform brightness.<br />

This definition is merely statistical <strong>and</strong> does not imply anything about <strong>the</strong> true distribution <strong>of</strong> shapes <strong>and</strong><br />

sizes <strong>of</strong> bright or dark regions. However, it has recently been found that <strong>the</strong> well-known <strong>and</strong> proven<br />

notion <strong>of</strong> "speckle size" is correct also with respect to <strong>the</strong> individual size <strong>of</strong> <strong>the</strong> bright spots [Fre96b].<br />

Even <strong>the</strong> intensity pr<strong>of</strong>iles <strong>of</strong> individual speckles have been found to follow <strong>the</strong> course <strong>of</strong> R I (∆x, ∆y) quite<br />

well [Fre96b, Fre98a], which means that <strong>the</strong>re is only a very small region <strong>of</strong> quasi-constant intensity<br />

within a bright speckle; <strong>the</strong> greater <strong>the</strong> peak intensity, <strong>the</strong> greater will be <strong>the</strong> intensity gradient within <strong>the</strong><br />

speckle area.<br />

The derivation <strong>of</strong> (2.41) is based on a two-dimensional treatment <strong>of</strong> <strong>the</strong> Kirchh<strong>of</strong>f-Fresnel diffraction<br />

integral. It is possible to extend <strong>the</strong> calculation to find <strong>the</strong> three-dimensional autocorrelation [Leu90]. The<br />

general result is ra<strong>the</strong>r difficult an expression; however considering <strong>the</strong> z direction only, one finds for a<br />

circular aperture [Leh98]<br />

<strong>and</strong><br />

α ⎛ 2π<br />

i∆z⎞<br />

z<br />

µ A( ∆z)<br />

= exp⎜<br />

⎟ with α = 8λ<br />

2π<br />

i∆z<br />

⎝ α ⎠<br />

D<br />

⎛ ∆z⎞<br />

µ A( ∆z)<br />

= sinc⎜<br />

⎟<br />

⎝ α ⎠<br />

2<br />

2<br />

,<br />

(2.44)<br />

where sinc(x)=sin(πx)/(πx). The first zero <strong>of</strong> this expression, indicating <strong>the</strong> length <strong>of</strong> a correlation cell, is at

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