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

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62 3. <strong>Calibration</strong> <strong>of</strong> <strong>Terrestrial</strong> <strong>Laser</strong> <strong>Scanner</strong>Table 3.13:Results <strong>of</strong> the adjusting hyperbola concerning the error <strong>of</strong> the collimation axis in horizontal direction.Parameter a defines for the gradient <strong>and</strong> parameter b defines the limit.Data Series a[°/m] b[°] aa[°/m] *fe[°]sphere 12 cm (1) 0.064 -0.016 0.0025 0.0007sphere 12 cm (2) 0.049 -0.016 0.0022 0.0006sphere 15 cm (1) 0.046 -0.014 0.0007 0.0002sphere 15 cm (2) 0.038 -0.014 0.0034 0.0010with the ranges <strong>and</strong> the difference tp <strong>of</strong> the horizontal directions in two faces corrected by the tw<strong>of</strong>oldcollimation error. The resulting values for the eccentricity are summarized in Figure 3.35. The eccentricitye can be described by a mean value <strong>of</strong> 0.9 mm <strong>and</strong> a precision <strong>of</strong> 0.1 mm. The mean value is based on dataup to 15 m because the influence <strong>of</strong> the eccentricity decreases <strong>and</strong> then reaches the same degree <strong>of</strong> precisionas the precision <strong>of</strong> the angle measurement system, cf. Table 3.12.2.0eccentricity (horizontal component)>| 0.0co>uo4> -10— 12cm (1)—15cm (1)—12cm (2)—15cm (2)"200 2 4 6 8 10 12 14 16 18 20range [m]Figure 3.35: Eccentricity <strong>of</strong> the collimation axis in horizontal direction. The eccentricity <strong>of</strong> the collimation axis inthe horizontal direction is derived by using spheres with the diameters <strong>of</strong>'12 cm <strong>and</strong> 15 cm based on two independentsetups (1) <strong>and</strong> (2).In summary, the error budget <strong>of</strong> the collimation axis, consisting <strong>of</strong> the collimation error <strong>and</strong> the eccentricity,was derived. Considering the influence <strong>of</strong> both errors shown in Figure 3.34, it can be seen that the adjustinghyperbolaeintersect the abscissa. This means at the intersection point, about 3 m to 4 m), the error <strong>of</strong> thecollimation axis has no influence on the horizontal direction. The interpretationis the collimation error <strong>and</strong>the eccentricity have opposite signs <strong>and</strong> they compensate each other. However, the most important aspectis that the influence <strong>of</strong> the error <strong>of</strong> the collimation axis is not constant for close ranges. The correction <strong>of</strong> thehorizontal angle data has to be completed separately according to the range <strong>and</strong> its error budget.Vertical ComponentSecond, the component in vertical direction is discussed. The results obtained by the two independentsetups are shown in Figure 3.36. It can be seen that the results <strong>of</strong> each setup obtained by the two sphereswith different diameters match each other.However, the results <strong>of</strong> the two independent setupseach other. With the exception <strong>of</strong> the first two meters, no systematic effects, depending on the range,do not fitcan beseen. The lines approximately describe a constant line. Thus, a significant influence <strong>of</strong> an eccentricity <strong>of</strong> thecollimation axis in the vertical direction cannot be seen. The constant line defines a collimation error in thevertical direction, which can be interpreted as an index error in the vertical encoder. Further assumptions<strong>of</strong> the factors that influence the orientation <strong>of</strong> the laser beam concern an <strong>of</strong>fset between the outgoing laserbeam <strong>and</strong> the encoder readings,variations on the rotation time <strong>and</strong> wobble effects <strong>of</strong> the horizontal axis.

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