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Application and Optimisation of the Spatial Phase Shifting ...

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146 Improvements on SPS<br />

Finally, both (6.5) <strong>and</strong> (6.8) were checked for <strong>the</strong>ir spectral transfer properties by means <strong>of</strong> bsc(ν x ). With<br />

<strong>the</strong> same input interferograms <strong>and</strong> averaging <strong>of</strong> <strong>the</strong> same portions <strong>of</strong> <strong>the</strong> bsc(ν x ,ν y ) maps as in 3.4.5, this<br />

gives <strong>the</strong> plots shown in Fig. 6.10.<br />

1.57<br />

1.57<br />

0.785<br />

0.785<br />

0<br />

0 1 2 3 4<br />

0<br />

0 1 2 3 ν x /ν 0x 4<br />

ν x /ν 0x<br />

-1.57<br />

-0.785<br />

-0.785<br />

-1.57<br />

Fig. 6.10: Left: bsc(ν x ) for (6.5); right: bsc(ν x ) for (6.8).<br />

By comparison with <strong>the</strong> graphs in Fig. 3.33 <strong>and</strong> Fig. 3.36, it can be seen that <strong>the</strong> noise has got higher; but<br />

for (6.8), <strong>the</strong> region <strong>of</strong> low detuning errors is distinctly increased as compared to (6.5). However it was<br />

found that <strong>the</strong> phase error δϕ O (∆ϕ) (cf. Fig. 5.4) produced by (6.8) has small maxima at ∆ϕ=π/2 <strong>and</strong> 3π/2<br />

(cf. Fig. 3.39), which indicates that δϕ O due to phase-shift errors is suppressed less efficiently when <strong>the</strong><br />

intensity correction is used.<br />

6.3 Modified phase shifting geometry<br />

If we use a circular aperture with a phase shift α x only, <strong>and</strong> if <strong>the</strong> measuring points are arranged as in Fig.<br />

3.26, we discard <strong>the</strong> phase information that would be accessible via <strong>the</strong> vertical coherence length <strong>of</strong> <strong>the</strong><br />

speckles. But due to <strong>the</strong> general shortage <strong>of</strong> spatial coherence in our small-speckle patterns, we should use<br />

it as exhaustively as possible. During <strong>the</strong> comparison <strong>of</strong> different phase retrieval approaches that will be<br />

described in this subsection, <strong>the</strong> σ d refer to just two sets <strong>of</strong> interferograms, namely a tilt series with B=3<br />

when intensity correction is involved, <strong>and</strong> ano<strong>the</strong>r with B=30 when it is not. In both cases, N x ∈ [0, 100]<br />

<strong>and</strong> d sx = 3 d p .<br />

Provided a frame-transfer or line-transfer camera with progressive scan readout is available, all image<br />

lines can be acquired simultaneously. Then it is possible to introduce an additional vertical phase shift α y<br />

by simply shifting <strong>the</strong> origin <strong>of</strong> <strong>the</strong> reference wave to (∆x,∆y). This results in a slant <strong>of</strong> <strong>the</strong> carrier fringes<br />

<strong>and</strong> allows to choose any desired direction for <strong>the</strong> set <strong>of</strong> pixels to use. Examples <strong>of</strong> composite phase<br />

shifting have been given in [Küch91, Küch97] for classical <strong>and</strong> in [Wil91] for speckle interferometry.<br />

When <strong>the</strong> speckle shape can be fully exploited for measurement, <strong>the</strong> measurement's accuracy should<br />

improve, since <strong>the</strong> ideal situation <strong>of</strong> Fig. 3.26, where all <strong>the</strong> used pixels are inside <strong>the</strong> same bright speckle,<br />

is unlikely to occur. More <strong>of</strong>ten, speckle "boundaries" are crossed, which results in an unreliable phase<br />

measurement. To diminish <strong>the</strong> noise, it should help to include <strong>the</strong> possibly better data <strong>of</strong> <strong>the</strong> orthogonal<br />

direction <strong>and</strong> to establish an averaged phase value.

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