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Application and Optimisation of the Spatial Phase Shifting ...

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56 Electronic or Digital Speckle Pattern Interferometry<br />

calculated ∆ϕ /rad<br />

6.28<br />

4.71<br />

3.14<br />

1.57<br />

0<br />

difference <strong>of</strong> phases<br />

phase <strong>of</strong> differences<br />

0 1.57 3.14 4.71 6.28<br />

pre-set ∆ϕ /rad<br />

measured ∆ϕ /(π/128)<br />

256<br />

224<br />

192<br />

160<br />

128<br />

96<br />

64<br />

32<br />

0<br />

difference <strong>of</strong> phases<br />

phase <strong>of</strong> differences<br />

0 100 200 300 400<br />

x/sensor column<br />

Fig. 3.3: Left: calculated ∆ϕ , averaged over ϕ O , vs. pre-set ∆ϕ , for <strong>the</strong> methods to be compared in this subsection.<br />

Right: measured pr<strong>of</strong>iles <strong>of</strong> vertical sawtooth fringes, averaged over 200 rows.<br />

Evidently, <strong>the</strong> phase-shifting method is not directly applicable to speckle correlation fringes. It will only<br />

work acceptably if <strong>the</strong> individual speckle phases are suppressed, i.e. <strong>the</strong> secondary interferograms must be<br />

smoo<strong>the</strong>d to approximate <strong>the</strong> cosinusoidal envelope <strong>of</strong> (3.20) as closely as possible. This is usually done<br />

by a low-pass filter <strong>and</strong> reduces <strong>the</strong> spatial resolution.<br />

The left-h<strong>and</strong> part <strong>of</strong> Fig. 3.4 shows <strong>the</strong> fringe pr<strong>of</strong>ile plotted in Fig. 3.3 on <strong>the</strong> right: surprisingly, <strong>the</strong><br />

image does yield direction information, although <strong>the</strong> averaged fringes do not. The reason is that for<br />

π/4< ∆ϕ

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