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Figure 2. Amplitude correction by fitting a polynomial. Top:The original amplitude plotted against range
Figure 3. Amplitude correction using range binning andcorrection by binned means. Top: Original amplitudedistribution with bin centres as blue line
Figure 5. Top: Distribution of the original amplitude over rangefor all spheres on all plots
Figure 7. 3D plot of a single scan point cloud. The circularstructure in the centre without points is the location of thescanner

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