Full text: Proceedings, XXth congress (Part 3)

   
    
       
    
   
         
   
   
   
     
  
method of the 
same direction 
the opposite 
cantly smaller 
slopes (i.e. to 
ted for every 
it strips. The 
mode derived 
h building and 
c.f. Table 8. 
International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV, Part B3. Istanbul 2004 
  
  
Direction 2F- 3F- 4F- SF- 6F- 
of edge RTK RTK RTK RTK RTK 
  
ACTOSS 34x13 21:16 18:49 | -30+38 217 
  
  
  
  
  
  
  
  
  
Along 77 15:43 14x11 24412 13:9 
Oblique 19:46 31331 34+25 27328 | 21:49 
Total 20:37 27426 26:3] 13436 19:38 
  
  
  
Mean 
difference 
  
11.6 96 
Table 9. Mean differences (cm) and standard deviations of the 
roof lengths from first pulse mode observations and 
RTK measurements. 
The mean difference of the roof lengths across the flight strip 
number 5 (first pulse) is negative. In this case, the laser 
observations from the edge of some roofs were not accepted to 
the roof plane because their undulations were too big. Hence 
the roofs became shorter than in reality. The along flight strip 
results for the first pulse mode observations (7-24 cm) are 
expected to be smaller than the across flight strip results (18-34 
cm) because of the scan pattern. The standard deviations were 
quite small, between £3-12 cm. In total the roof lengths from 
the first pulse mode are about 21 cm longer than the reference 
lengths from RTK measurements. 
  
  
14.0 % 
Direction 2L- 3L- 4] ~ SL- 6L- 
ofedge RIK RIK RTK RTK RTK 
  
ACTOSS -52+30 | -40+11 -26x8 -81+13 -29+5 
  
Along =35132 | 432 | 2721 | -32422 | 4723 
  
Oblique -18+31 -9+39 -7+23 -12+16 | -1328 
  
  
4.4 % 
  
Total -29433 | -21x36 | -19+23 | -32+33 | -23425 
  
  
  
  
  
  
  
  
13.2 % 
  
11.4% 
  
  
  
the last pulse 
latively small 
ulse measured 
(4.4 %) when 
s flat or pitch 
at were lower 
> observations 
systematically 
neasured roof 
with the laser 
lengths were 
anes. Because 
rn the lengths 
1e flight strip, 
. The distance 
ction is about 
> flying height 
»verlap on the 
Table 10. Mean differences (cm) and standard deviations of the 
roof lengths from last pulse mode observations and 
RTK measurements. 
The last pulse mode results in Table 10 for the along track 
direction do agree with the relation depicted in Table 9 between 
across and along track directions. Again the across track value 
(-81 em) of the flight strip number 5 indicates the shortest roof 
lengths. In total the roof lengths from the last pulse mode are 
about 25 cm smaller than the reference lengths from RTK 
measurements. 
4. DISCUSSION 
The obtained elevation accuracy for repeated strips was good. 
Also planimetric errors were mainly detected by comparing 
strips flown with opposite directions. 
The mean height errors for elevation points were —2 to +1 cm 
and standard deviations were mainly +3-4 cm and for one strip 
it was £9 cm. These values are comparable to other previous 
results for planar targets (e.g. Ahokas et al., 2003). 
Centre points and ridges of the extracted buildings were used to 
test how small planimetric changes in the laser data affect the 
obtained building model. Therefore, we also indirectly analyzed 
the accuracy of the building extraction model. In paper by 
Rónnholm (2004), a similar description of the systematic 
internal quality of repeated measurements using point cloud 
data is given. 
The mean distances between the centre points of the buildings 
derived from the first and last pulse observations differed less 
than 20 cm from each other while the standard deviation was 
+9-16 cm (Table 6). In one flight strip these errors include the 
building extraction modelling errors and the errors resulting 
from the differences between the first and the last pulse data. 
Normally the shape of the building was the same, only area was 
changed. When we compared the mean distances between the 
centre points of the laser derived buildings and buildings on the 
map, less than 30 cm differences occur. Standard deviations 
were £11-28 cm and +14-18 cm (Tables 4 and 5). These mean 
errors include the building extraction modelling errors, the 
systematic shift between the transformed map and laser 
coordinates and also the along track shift of the laser 
observations to the fight direction. This gives information how 
well the buildings can be extracted in real life from laser 
scanner data. Vógtle et al. (2000) reported that the interior 
accuracy of the modeled buildings is about 420-30 cm in 
position and £5-10 cm in elevation. When they compared the 
wireframe model with the manually derived CAD model the 
coordinate differences were about +20-90 cm in xy and about 
+20 cm in z. Steinle et al. (2000) reported the differences 
between the first and last pulse derived wireframe models. In 
this case the first and last pulse flights were from different dates 
and the grid size was 1x1 m?. Mean differences were about 0.8- 
1.5 m in xy and about 0.2-0.6 m in elevation. 
First and last pulse data give different results for building sizes. 
The total mean differences of roof lengths from first and last 
pulse varied from about —30 to +30 cm and the standard 
deviation was less than +40 cm (Tables 9 and 10). Buildings 
were of different size and orientation. Some errors are by 
inheritance from the observation geometry of the Toposys ALS. 
An internal precision of 10-20 cm for dimensions of 10 
buildings was reached in a study of Maas et al. (1999). The 
FLI-MAP system produced a point density of 5 points/m°. 
The results showed that the same ridge can be extracted by 
repeated measurements with less than 3-5 cm systematic error 
and the standard deviation of the shifts between acquisition was 
less than 5 cm when using strips flown in the same direction. In 
general this implies that the ridges extraction is very accurate 
and the repeatability of the laser scanning with Toposys Falcon 
is good. 
5. CONCLUSIONS 
The repeated observations of five Toposys Falcon flight strips 
from Espoonlahti area were compared with each other and with 
reference data. 
Using reference measurements, the systematic height errors for 
elevation points were —2 to +1 cm and standard deviations were 
mainly +3-4 em. It can be concluded that the changes in height 
errors of these five strips is negligible. 
In planimetry, mean distances of the centre points of the 
buildings were less than 30 cm for the first and also for the last 
pulse data when compared with the buildings on the map. The 
standard deviations varied between £11-28 cm (first pulse) and 
+14-18 cm (last pulse) in different flight strips. The planimetric 
accuracy of the object (building) on the ground depends on the 
direction of the flight. There is an along track shift of about 5 
cm to the flight direction. The accuracy obtained using the 
centre points of the buildings depends on the extraction 
accuracies and the distribution of the laser points on the ground. 
Results obtained using the ridges confirmed that there is a 
difference in planimetric accuracy between the flight strips to 
the opposite direction and to the same direction. Biases were 3- 
5 cm and standard deviations +3-5 em for the flight strips to the 
   
   
   
   
   
   
      
   
   
      
   
   
    
    
   
  
   
   
     
  
  
  
  
   
   
   
   
    
    
    
    
     
     
    
   
    
     
  
    
	        
Waiting...

Note to user

Dear user,

In response to current developments in the web technology used by the Goobi viewer, the software no longer supports your browser.

Please use one of the following browsers to display this page correctly.

Thank you.