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Table 2. Cyrax and Optech laser scanner specifications
MANUFACTURER
Cyra Technologies || Optech Inc.
PRODUCT HDS2500 ILRIS-3D
PERFORMANCE
Laser Wavelength (in nm) 522 1540
Laser Power (in W, mW) « | mW avg 10 nàV
FDA Laser Classification (Class) 2 Cas var gerne mes
Beam Diameter at Specified Distance x6 mm from € | 0675 in at lon
(0.Y ft at X ft/Ymm at X m) 50m 1/17 mm at 30 m
Measurement Téchnique Time of flight | LDA (Time of Flight
Average Data Acquisition Rate (pps) 1,000 2,009
.Maximum Data Acquisition Rate (pps) 1,000 3,000
Distance Accuracy at Specified Distance
(O.Y ft at X ft/Ymm at X m)
Position Accuracy at Specified Distance
(0.Y ft at X ft/Ymm at X m)
Angular Accuracy
0.275 in of 330 1/7
mm at 100m, [2]
14 in at 330 ft/10
mm at 100 m, [2]
€0 micro-radians | (9 eges Caco 3
4 mm at 50m
4 mm at 50m
Minimum Range (feet/m) 15 m 10/5 m
Maximum Range (feet/m) 100 m NEO R> 1,506 pic]
Field of View (vertical angle) 40 degrees [8j
Field of View (horizontal angle) 40 degrees | Pen Asp
GENERAL
Scanner Dimensions (LxWxH) hia xan {1200 IIS BIE]
Scanner Weight (pounds/kg) 20.5 kg 25 Ibs/12 ke
4. THE 3D MODELING
As previously mentioned, the Scrovegni Chapel was chosen for
this project because of its simple architecture: the presence of a
single hall (nave) allowed us to survey the interior with case
without occlusions of the walls and the vaulted ceiling.
Conversely, the apse has revealed to be more tricky to be
completely surveyed given the presence of the main altar,
which made impossible to scan some parts of the walls, given
the small room available between the back of the altar and the
apse. This area resulted in a wide hole in the 3D model that had
to be manually closed using both artificial surface patches and
a few digital images as reference guide for the hole filling
stage.
Since all employed laser sensors were able to acquire the
intensity of the reflected beam, figures of the paints were
imaged on the point clouds, as well. Such features could be
often well recognized on the intensity data and therefore
extensively used as reference points during the alignment
procedure, as described in following subsection.
Prior to registering the scans, the range data were linearly
interpolated in order to get a uniform point spacing, since they
were acquired with different resolutions: 8mm for Mensi and
Optech, 35mm for the Cyrax and ! em for Riegl. Accordingly a
8mm grid size was chosen as a trade-off between point cloud
density and size of related data files being processed. However
the interpolation was applied to Cyrax data only, while Riegl
scans were left unchanged to avoid the addition of artificial
(i.e. not real) points in the corresponding clouds. All the
processing steps were carried using Polyworks [Innovmetric
inc.] a powerful 3D modeling software which allows to work
with multiresolution range data.
Then a 2 steps interactive manual N-points alignment
procedure was adopted to register the scans with each other:
matching points were easily recognized using only the intensity
data, as shown in figure 3. As most part of the church was
surveyed by the Mensi laser scanner, (95% of the hall and 10%
of the apse), related scans were used as main data block for the
registration, at this stage.
International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV, Part BS. Istanbul 2004
Figure 3. Interactive manual alignment.
After all the scans were manually aligned, a global ICP-based
registration algorithm was applied in order to refine the results
of previous step. Such approach [Soucy et al, 1996] yielded a
very good registration for the Mensi scans, with an average
RMS alignment error of 0.006 m, confirming the goodness of
the registration procedure implemented in Polyworks: the
residual error is due to the inherent accuracy of the laser
scanner. However, if remaining scans of the Cyrax, Optech and
Riegl laser scanners are taken into account, then the RMS
grows to about lcm, as showed in figure 4. This increase could
be explained considering that, among employed laser sensors,
the Riegl was the noisiest and related scans were used to join
the range data from the nave (surveyed mainly with the Mensi)
with the ones from the apse (completely surveyed by the Cyrax
only).
An example of the comparison of noise content between range
data of Riegl, Optech and Mensi laser scanners is presented in
figures 6 b-d, which relate to the survey of the surface of the
wall displayed in figure 6a.
*; IMAlign - Alignment &t
Parameters Statistics | Comparison
# lterations
33
Convergence
indx Conv Mean .StdDev
46 3.0e-008 0.529448 10.14501 a
47 30e-006 2404396 6.263409
48 3.0e-008-0.356729 7.671836
49 3.0e-008-0613273 12.56912
50 3.0e-008 0.353304 12.53452
51 3.0e-008 1.313603 10.47731
52 3.0e-008 1.939209 9.818244
53 3.0e-008 0.840151 11 27706
54 8.2e-010 0.316092 8.916086
55 82e-010-0.218566 11.26402
56 &Ce-010 0.180667 10.791569
5? 82e-010-0 252367 4242511
58 7.0e-011 0.777804 5.659035
59 7.0e-011 0.545312 7.084582 x]
c^ 010 ^43 PARAM AR TAC An Ar
Start | Close
Figure 4. Results of global alignment