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Application and Optimisation of the Spatial Phase Shifting ...

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6.2 Modified phase reconstruction formulae 145<br />

0.12<br />

σ d /λ<br />

0.10<br />

0.08<br />

0.06<br />

0.04<br />

0.02<br />

0.00<br />

3-sample 90°, B=30<br />

3-sample 90° with intensity correction, B=3<br />

3+3-sample averaging 90°, B=30<br />

3+3-sample averaging 90° with intensity correction, B=3<br />

0 20 40 60 80 N x 100<br />

Fig. 6.9: Overview <strong>of</strong> σ d from ESPI displacement measurements as a function <strong>of</strong> N x , obtained with various phase<br />

calculation formulae from two series <strong>of</strong> interferograms: without intensity correction, B=30 (black<br />

symbols); with intensity correction, B=3 (black symbols filled white); 3-sample formulae, triangles; 3+3-<br />

averaging formulae, squares.<br />

The summary presented in Fig. 6.9 allows some conclusions: (i) <strong>the</strong> use <strong>of</strong> a 3+3 averaging scheme alone<br />

is definitely a better choice than an intensity-error compensating formula alone. (ii) The combination <strong>of</strong><br />

both error-reduction methods leads to <strong>the</strong> lowest overall error; at d s =3 d p , σ d remains below λ/20 up to<br />

N x =20. (iii) Introducing <strong>the</strong> intensity-error correction effects indeed a slightly greater improvement in σ d<br />

when a phase-shift error elimination is already present, <strong>and</strong> vice versa. (In o<strong>the</strong>r words, <strong>the</strong> lower two<br />

curves are far<strong>the</strong>r apart than <strong>the</strong> upper two.) This confirms <strong>the</strong> initial presumption that motivated this<br />

subsection: <strong>the</strong> two methods pr<strong>of</strong>it from each o<strong>the</strong>r if used toge<strong>the</strong>r. However, as mentioned before, in<br />

most practical cases it will suffice to set B30 <strong>and</strong> to do without <strong>the</strong> small benefit <strong>of</strong> <strong>the</strong> intensity<br />

correction, all <strong>the</strong> more since this speeds up <strong>the</strong> calculations considerably <strong>and</strong> even makes <strong>the</strong>m accessible<br />

to <strong>the</strong> use <strong>of</strong> look-up tables.<br />

Finally, it may be worth noting that a 3+3 averaging formula according to [Bur98a]<br />

ϕ ' mod π = arctan<br />

O<br />

K2 + K5<br />

− K + K − K + K<br />

1 3 4 6<br />

(6.9)<br />

is error-compensating only by averaging, but does not eliminate <strong>the</strong> cyclical errors shown in Fig. 3.39,<br />

since it constitutes <strong>the</strong> average over ϕ O <strong>and</strong> ϕ O +90°. Hence, (6.9) will do little more for error reduction<br />

than <strong>the</strong> intensity correction without averaging, which means that even <strong>the</strong> pure phase-shift error<br />

compensation <strong>of</strong> (3.56) would perform better. This was in fact found in [Bur98a], where (6.9) was used<br />

instead <strong>of</strong> (6.8), <strong>and</strong> emphasises <strong>the</strong> relevance <strong>of</strong> an optimal composition <strong>of</strong> <strong>the</strong> averaging formula.

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