Things to keep in mind while scanning
- Get excellent data to work with
Things to keep in mind while scanning - Get excellent data to work - - PowerPoint PPT Presentation
Things to keep in mind while scanning - Get excellent data to work with Richard Steffen Martin Graner CTO R&D Engineer Table of contents 1. Project planning 2. Scanning 3. Registration 2 Things to keep in mind - 2020 Table of
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Beam Divergence Spot Size Distance ----------------------------------------------- >
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Single Point Accuracy Distance ----------------------------------------------- > ςα ςd ςα = const (Faro 19 arcsec = 0.005°) ςd = const + ppm (Faro 1mm + 10 ppm)
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Things to keep in mind - 2020
○ Reflected waveform has multiple peaks in time diagramm ○ Usually mean will be computed (ghost points on edges)
○ Should be considered in the adjustment ○ Should be considered in distance measurements
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C2C Feature based Matching via:
Limits:
existing (e.g. long hallways)
Gets time consuming when:
the connection graph) Manual Topview pre-alignment
values Constellation search:
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Scan: Scan connection
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Scan: Scan connection
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Loop closure Scan:
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Loop closure Scan:
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Feature distribution Feature: Scan:
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The good Feature: Scan:
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The bad Feature: Scan:
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The ugly Feature: Scan:
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The super bad luck
60° 60° 60°
Feature: Scan:
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The super bad luck Feature: Scan:
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The super bad luck Feature: Scan:
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The super bad luck Feature: Scan:
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Door scanning Configuration 1
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Door scanning Configuration 2
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Source: https://www.laserscanning-europe.com/en/news/use-laser-scanner-reference-spheres-optimal-distance-to-the-scanner
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○ Which Scans are overlapped (adjacency matrix) ○ Which local features correspond to each other (constellation search)
○ Complexity O (n2 / 2) ○ Clustering 20->100 Scans per cluster
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○ Xw Unknown 3D Position ○ Xlocal Measured local 3D Position
○
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○ The model: X2 = ΔH12 X1 (Helmert transformation between 2 scans) ○ Cloud 2 Cloud use IPC to detemine ΔH12
○ The model: Hw2 = ΔH12 Hw1 (Relative orientation)
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