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Calibration of a Terrestrial Laser Scanner - Institute of Geodesy and ...

Calibration of a Terrestrial Laser Scanner - Institute of Geodesy and ...

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'94 5. Kinematic <strong>Laser</strong> Scanningbeam is not punctiform, but has a more complex structure during propagation in the air, cf. Section 2.1.2.If the laser beam hits an object, a footprint <strong>of</strong> the laser beam is generated.Therefore, the 'real' footprintis much larger than the 'visible' footprint. Furthermore, the sensitivity <strong>of</strong> the diodes is important. Only asmall part <strong>of</strong> the laser beam needs to hit the photo diode to start the process.If another part <strong>of</strong> the laserbeam hits the photo diode directly a second time, the stopping process is performed.Neither does the laserbeam rotate 2tt nor can a reproducible <strong>and</strong> reasonable rotation time T be derived. To avoid these problems,either a more complex electronic circuit has to be developed or two photothem have to be implemented. The latter was used in this study.diodes with a distance betweenThe use <strong>of</strong> two photo diodes implicates some specialties with respect to the experimental setup. Addition¬ally, the center angle a has to be determined. Referring to the postulation regarding the precision<strong>of</strong> therotation time T, the required precision for the center angle a can be estimated. To achieve the best possibleprecision for the center angle a, the principle<strong>of</strong> autocollimation was used. InFigure 5.4, the two photodiodes, as well as the autocollimation mirror mounted on a plate, can be seen. This plate can be aligned byan adjusting device.autocollimationmirrordiode(stop)centre laser beam(rotating mirror]diode(start)Figure 5.5: Mathematical relations for deriving the center angle a: the radius r,be known.the base b <strong>and</strong> the <strong>of</strong>fset Ar has toIn Figure 5.5, the mathematical relation between the desired center angle a, the plate including the photodiodes, <strong>and</strong> the autocollimation mirror can be seen. The center angle a can be caluclated bya = 2 •arctan-2(r Ar)(5.5)where r is the radius, i.e.distance between center <strong>of</strong> rotating mirror <strong>and</strong> autocollimation mirror, Ar is the<strong>of</strong>fset between the photodiodes <strong>and</strong> the autocollimation mirror <strong>and</strong> b is the base i.e.the distance betweenthe two diodes. The <strong>of</strong>fset Ar was measured with a slide gauge several times. As result, the <strong>of</strong>fset Ar is lessthan 0.5 mm with a precision <strong>of</strong> about 0.1 mm. Considering Equation (5.5), the influence <strong>of</strong> Ar is negligible,if the radius r is larger than 0.5 m. The reason is that, assuming the slowest angular freqeuncy <strong>of</strong> 12.5 rps2,the influence on the rotation time T is less than the time precision <strong>of</strong> 1/xs claimed. Thus, Equation (5.5)simplifies to a = 2 •arctan2r(5.6)2Rps: rotations per second. According to the specifications <strong>of</strong> the manufacturer, there are three different rotating velocities: ojns12.5rps(Tfa0.08s),w25 fa 25rps (T fa 0.04 s) <strong>and</strong> w33 fa 33 rps (T fa 0.03 s)

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