International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV, Part BS. Istanbul 2004
E Control p
Figure 7 Mosaic of rectified photographs in the wall of the
nave of St. Domingo de Silos’ Church (4mm
GSD). Photographs taken with the 20 mm lens are
also shown. Control and check point network is
displayed.
In this case, only one strip (10 parallel photographs plus two
convergent ones) was processed. Camera stations were at 9.5
m, as average, from the wall and the bases were 1-1.2 m, so
the B/D ratios were near to 1/10.
WALL A B
rms XY +56 mm X52 mm
max. Vxy (abs.) 69 mm 6.4 mm
rms Z 79 mm +71 mm
max Vz (abs.) 12.3 mm 13.8 mm
Prop. Error (XY) 1:2500 1:2650
Prop. Error (Z) 1:1200 1:1400
Table3 . Wall case. A: rms and proportional errors in
planimetry (XY) and depth (Z) at check points
with the camera pre-calibrated. Maximum
residuals in XY and Z (in absolute values) are
also expressed. B: rms and proportional errors in
(XY) and (Z) at check points after field self
calibration.
Control, check and pass points were measured and, then, the
strip triangulation was processed considering the camera
calibrated at the laboratory conditions. Next, a new run with
self calibration was carried out and inner parameters were
also adjusted. The results are displayed in Table 3. In this
table, the proportional errors in XY and Z are also expressed
as rmsxy with respect to largest distance in the wall
(approximately 14 m) and rmsz with respect to the camera-
object distance (9.5 m).
In case A (Table 3A) with the camera calibrated at
laboratory, accuracy was similar to that of the vault case
(mean errors below +8 mm). But, the field self calibration did
not improve meaningfully the accuracy, just nearly 10 % in
both XY and Z (Table 3B). In any case the final results met
the accuracy requirements (+ 3 cm in coordinates and a final
plotting scale of 1:50). Probably, the photogrammetric
network in this case was not strong enough to solve
adequately the self calibration.
4.3 Comparison of UMK stereopairs and analytical
plotter with Canon D30 in the study of a facade
Finally, another usual situation in architectural
photogrammetry has been tested. In this case, single Canon
D30 stereopairs have been oriented and the results have been
compared to those obtained with a metric camera (UMK
1318/10) and analytical stereoplotter (Leica SD-2000),
(Figure 8).
Figure 8 Two UMK 1318/10 stereopairs (above) and two
Canon D30, with 20 mm lens (below), in the
façade of St. Domingo de Silos’ Church.
The church façade was photographed with the UMK and two
stereopairs were taken. Usual 1/5 B/D ratios were employed
and the photo scales were approximately 1:100. The
orientations were made with 12 parallax points per model
(distributed as usual in six areas), 4 control points per model
and a total of 8 check points. Table 4 displays a resume of
the accuracy obtained in both UMK stereopairs. Errors are
better than + 5 mm. These errors were the expected with
these data acquisition and reduction methods since the
control point were well defined but natural points. The
orientation errors with the Canon D30 were compared with
these data.
Stereopairs with the Canon D30 were taken with same
conditions. All points were manually measured and a bundle
adjustment was performed. But orientations were computed
in six different ways. First, the models were solved same as
the UMK stereo pairs by using the field control points
(Canon D30 CP in Table 4). Although accuracy has been
poorer than in the UMK case (as expected), good results
were obtained with mean errors better than + 1 cm. In this
case the camera was considered as calibrated (with data of
Table 1) since self calibration was not possible in single
stereopairs.
A second choice was selected since it is usual the lack of
control points in fast and low cost surveys. In this case
stereopairs were oriented with a known distance (DIST in
Table 4) and three selected points for datum definition
(Atkinson, 1996).
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