07.11.2014 Views

Application and Optimisation of the Spatial Phase Shifting ...

Application and Optimisation of the Spatial Phase Shifting ...

Application and Optimisation of the Spatial Phase Shifting ...

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

124 Comparison <strong>of</strong> noise in phase maps from TPS <strong>and</strong> SPS<br />

The sensitivity vector lies in <strong>the</strong> object's plane in horizontal direction; in this case, only x-displacements<br />

can be measured. The object rotation generates 1.4 horizontal sawtooth fringes per wavelength <strong>of</strong> in-plane<br />

displacement. Consequently, <strong>the</strong> conversion factor from phase to displacement is λ/509° or λ/(362 grey<br />

levels), which is approximately halfway between <strong>the</strong> out-<strong>of</strong>-plane <strong>and</strong> <strong>the</strong> in-plane sensitivity that we have<br />

previously been dealing with. (It would however be easy to increase this value: if both incidence angles<br />

were 53°, as in 5.5.1, we would get 1.6 sawtooth fringes per wavelength <strong>of</strong> displacement.) The<br />

measured σ d are shown in Fig. 5.10.<br />

σ d /λ<br />

0.20<br />

0.18<br />

0.16<br />

0.14<br />

0.12<br />

0.10<br />

0.08<br />

0.06<br />

0.04<br />

0.02<br />

0.00<br />

0 5 10 15<br />

20 30 40 50<br />

60 70 90 100<br />

0 2 4 6 8 d s /d p 10<br />

N y<br />

Fig. 5.10: σ d for ESPI displacement measurements with pure in-plane TPS as a function <strong>of</strong> speckle size for inplane<br />

displacements. The parameter for each curve is N y , <strong>the</strong> number <strong>of</strong> horizontal fringes per 1024<br />

pixels, as indicated in <strong>the</strong> legend box.<br />

Again, <strong>the</strong> ordinate reflects <strong>the</strong> change in sensitivity: σ d,max 0.20 λ for this geometry. But since only 57%<br />

<strong>of</strong> <strong>the</strong> displacement <strong>of</strong> 5.5.1 are necessary to generate <strong>the</strong> same number <strong>of</strong> fringes, <strong>the</strong>re is less speckle<br />

decorrelation present than in Fig. 5.8. This improves <strong>the</strong> performance significantly for higher fringe<br />

densities, although <strong>the</strong> optimum <strong>of</strong> <strong>the</strong> speckle size still w<strong>and</strong>ers towards two or more pixels for larger<br />

rotations. Over <strong>the</strong> whole range <strong>of</strong> fringe densities, <strong>the</strong> accuracy is comparable to that obtained in <strong>the</strong> out<strong>of</strong>-plane<br />

TPS study. Apart from <strong>the</strong> comparison with SPS that we are to continue, this shows that specklereference<br />

ESPI is not very much inferior to <strong>the</strong> smooth-reference configurations <strong>and</strong> that a 3-D TPS<br />

system with Cartesian sensitivities would have well-balanced systematic σ d in each <strong>of</strong> <strong>the</strong> directions.<br />

5.5.3 Purely in-plane sensitive interferometer for SPS<br />

A set-up that facilitates exclusive in-plane displacement detection also with SPS has been described in<br />

[Sir97a]. Because <strong>the</strong> sensitivity <strong>of</strong> this configuration is also adjustable, we are able to compare <strong>the</strong> merits<br />

<strong>of</strong> SPS <strong>and</strong> TPS also with pure in-plane interferometers <strong>of</strong> equal sensitivity. Fig. 5.11 shows a schematic<br />

<strong>of</strong> <strong>the</strong> interferometer.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!