Full text: XVIIIth Congress (Part B1)

mean errors, 
rol points (4 
es) was also 
cantly. 
ufficient for 
er with 100 
es of digital 
ng 1:40,000 
1 orthoimage 
| pixel size). 
f4m in the 
he 1:24,000 
> measuring 
le for many 
racy without 
  
  
  
  
  
  
  
  
  
  
  
  
  
  
  
  
  
an affine 
x absolute 
y 
4 | 151 
3 139 
0 159 
4 117 
2 105 
2 91 
os 56 
; 54 
) 51 
p 151 
0 129 
6 122 
177 
:; 138 
) 114 
  
  
  
st stage the 
adial lens 
on, and the 
acements in 
oints were 
ween these 
s as control 
ration were 
transferred 
"here an x- 
e residuals. 
The same procedure was repeated many times and the correction 
grids were averaged to reduce temporal noise, especially due to 
vibrations. For the Horizon four scans were averaged, for the 
other scanners two, except for the Arcus where only one scan was 
available. For the y-correction grid (modelling of tangential lens 
distortion) a similar procedure was used. In this case once an 
affine transformation and once a 7 parameter transformation 
(affine plus an x? term in y) was used. The x? term in y 
corresponds to the second order tangential distortion. By 
subtracting the residuals from the two transformations, we were 
left with the errors modelled by the x? term in y, and 
subsequently a y-correction grid in the scanner system was 
computed as for x. The x-grid was always used, the y-grid (called 
y-precorrection) is optional. Errors due to lens distortion are 
stable, so these correction grids do not need to be computed often 
(for the Horizon we applied the calibration using correction grids 
that were computed one year in advance). 
For the second stage of the calibration the crosses of the two 
border lines of the on-line plate were measured by LSTM and an 
affine transformation between these values and the reference 
values using all points as control points was computed. The y- 
residuals of this transformation were indicating the occurring 
errors at the two border lines. For the A4 scanners only one 
border line was imaged, so a similarity instead of an affine 
transformation was used. Since scanning is performed in one 
swath we can assume that no errors can suddenly occur in the 
interior of the CCD. Thus, the error at any point in the interior of 
the image can be bilinearly interpolated using the errors at the 
borders. This calibration stage is used to model the y-errors. They 
are mainly due to mechanical positioning. The part coming due 
to the tangential lens distortion can either be excluded by using 
the y-precorrection grid, or it can be modelled by using a 
transformation higher than the affine in the interior orientation. 
We used just a 7 parameter transformation (affine plus an x? term 
in y). This was sufficient for all scanners. The seventh parameter 
can be only determined, if 8 control points (fiducials) can be 
used. 
4.3. Geometric accuracy after calibration 
To check the validity of the calibration procedure we scanned the 
two plates simultaneously, i.e. the off-line plate was placed on 
top of the on-line and were fixed by tape to the scanner stage. 
This could be avoided, if we had designed the off-line plate such 
that it included the two border lines of the on-line plate with the 
dense crosses. Due to this procedure the crosses of the upper 
plate were naturally radially displaced, but this effect could be 
accommodated by the affine transformation. However, this could 
not happen with the two A4 scanners since the glass plates were 
not lying on the scanner stage and the radial x-displacement was 
asymmetric. The same problem occurred with the Mirage. This 
scanner has a dual lens system employing many mirrors 
(unfortunately the scanner representative did not want to or could 
not provide us with technical details). The x-residuals of the off- 
line plate revealed an asymmetry with respect to the centre of the 
scanner stage, thus indicating that the lens had an asymmetric 
position with respect to the CCD line. These x-errors for the three 
scanners could be reduced by using additional transformation 
terms (x? or xy) in the x-direction (see version 3 in Table 3). The 
scan of both plates was done twice except for the Arcus. The 
results of the two scans were similar and the average is shown in 
Table 3. Table 3 shows statistics of the residuals of the check 
17 
points of the off-line plate after calibration. 
Version 1 includes an affine transformation and y-precorrection. 
Version 2 includes the aforementioned 7 parameter 
transformation and no y-precorrection. Version 3 for the last 
three scanners is like version 2 but with an additional term (x? Or 
xy) in the x-direction. The results of the three last scanners are 
not optimal due to the aforementioned problem with the 
positioning of the glass plate and the dual lens system of the 
Mirage. Still with version 3 we get an accuracy of 6 - 10 jum. This 
is remarkable especially for the Mirage, which had a scan pixel 
size of 63.5 um. The results of the first two A3 scanners is more 
representative and show an accuracy of 4 - 7 um. The JX-610 
reaches an accuracy similar to that of many photogrammetric 
scanners. Version 2 is slightly better than version 1 and does not 
require y-precorrection, so it is faster. The errors in x- are slightly 
larger than in y-direction, and have a remaining systematic part. 
The maximum errors are equal to 2.5 - 3.5 RMS. The achieved 
geometric accuracy corresponds to 0.1 - 0.2 pixels. If 8 fiducials 
and a 7 parameter transformation can be used, then no y- 
precorrection is necessary, while in all other cases the y- 
precorrection brings substantial improvement. 
Table 3. Statistical values (in Jum) of geometric accuracy after 
calibration indicated by the residuals of the check 
  
  
  
  
  
  
  
  
  
  
  
  
  
  
  
  
points. 
RMS | Mean | M^ 
Scanner | Version! Con SR 
points 
X YA | 
Horizon 1 4 8 8 4 1.0 22127 
2 8 7 6,13 1-9 | 20 | 20 
JX-610 1 4 7 61 5:15 [|:44 .|/16 
2 8 5 4 | 4 1 1414-1715 
Mirage 1 4 19 ]10:| 51 2. Fl 40] 23 
D-16L 2 8 14.1.8.11.-9.1..111.30.].22 
3 8 8 9 1 Lil 21.1722 
1 4 18] 11] 8 | -3148] 25 
Arcus II 2 8 16} 9.9] #4 [3139 [28 
3 8 10,19. 1,54. 1.3. 31. 22.1.28 
Power- I 4 1216 1-6 (1-1) 32 | 15 
Look 8 12; 15 6 agır=-S ch di {2330116 
3 8 10.)..6..1..0 1..].26 | 16 
  
  
  
  
  
  
  
  
  
  
  
! See explanation in text. 
Thus, calibration paves the way for use of DTP scanners in 
practically all photogrammetric applications, but at a cost: grid 
plates, development of calibration software, more computations 
for calibration and, if necessary, image resampling. 
4.4. Colour misregistration 
It was tested by scanning the resolution chart in colour and 
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B1. Vienna 1996 
 
	        
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