3D Time-of-flight distance measurement with custom - Universität ...
3D Time-of-flight distance measurement with custom - Universität ...
3D Time-of-flight distance measurement with custom - Universität ...
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OPTICAL TOF RANGE MEASUREMENT 13<br />
pr<strong>of</strong>ile can then be measured <strong>with</strong> one shot, and for <strong>3D</strong> data the scan only needs to<br />
be performed in one direction (light sheet triangulation). In industrial inspection<br />
applications, such a 1D scan is <strong>of</strong>ten available free <strong>of</strong> cost, since the objects to<br />
measure are moving anyway, for example on an assembly-line. [KRA] presents<br />
such a scanning <strong>3D</strong> camera working <strong>with</strong> active light sheet triangulation and<br />
delivering 50 depth images per second in CCIR video format.<br />
Further advanced techniques even use 2D structured light illumination and 2D<br />
imaging to perform <strong>3D</strong> triangulation <strong>measurement</strong>s <strong>with</strong>out scanning. The most<br />
important members <strong>of</strong> this structured light group are phase shifting projected fringe,<br />
Gray code approach [BRE], phase shifting moiré [DOR], coded binary patterns,<br />
random texture [BES] or color-coded light. They typically use LCD (Liquid Crystal<br />
Display) projectors for the projection <strong>of</strong> the structured patterns.<br />
Triangulation systems are available for applications from mm-range (depth <strong>of</strong> focus)<br />
to 100km range (photogrammetry). Their main drawback is that for a good<br />
resolution they have to be large in size, since they need a large triangulation base.<br />
On the other hand, the larger this triangulation base, the more they are restricted by<br />
shadowing effects. Also, <strong>3D</strong> triangulation systems are relatively expensive since<br />
they require fast LCD projectors (only active systems) as well as large<br />
computational power.<br />
2.1.2 Interferometry<br />
Interferometry is described by the superposition <strong>of</strong> two monochromatic waves <strong>of</strong><br />
frequency ν, amplitude U1 and U2 and phase ϕ1 and ϕ2, respectively, resulting in<br />
another monochromatic wave <strong>of</strong> the same frequency ν, but <strong>with</strong> different phase and<br />
different amplitude [SAL]. In the easiest interferometer setup, the Michelson<br />
interferometer, illustrated in Figure 2.3, a laser beam (monochromatic and<br />
coherent) is split into two rays by a beam splitter. One ray is projected to a mirror <strong>of</strong><br />
constant displacement x1 (reference path) whereas the other beam is targeted on<br />
the object <strong>of</strong> variable <strong>distance</strong> x2 (<strong>measurement</strong> path). Both beams are reflected<br />
back to the beam splitter, which projects them onto an integrating detector.