Full text: Proceedings, XXth congress (Part 3)

   
. Istanbul 2004 
| 3. Each flight 
  
International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV, Part B3. Istanbul 2004 
  
  
  
  
First | GFirst 
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+3 143 
  
  
  
) and standard 
alt and gravel 
ns. Results are 
st pulse data. 
The use of centres of buildings 
The distances between the laser derived building centre point 
and the corresponding centre point from the building map were 
calculated, as well as the distances between the centre points of 
buildings using the first pulse data and the corresponding 
buildings using last pulse data. Lines between opposite corner 
points of the extracted buildings determined the centre point of 
the building. Results are shown in Tables 4, 5 and 6. 
  
  
  
  
  
Last 6Last 
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) and standard 
it and gravel 
ns. Results are 
t pulse data. 
point area the 
-4 cm standard 
The decimetre 
oint method at 
es of buildings 
from the five 
in section 2.4. 
uildings could 
re grouped by 
^, double slope 
onnected ridge 
ridge roof type 
.g. ridge roof 
  
trip number 3 
ed buildings. 
  
  
Flight strip | 2F- 3F- 4F- SF- 6F- 
map map map map map 
Min dist. 7 4 9 | 4 
Max dist. 161 67 61 S3 69 
Mean +Std | 28428 23416 27:11 1812 24x15 
  
  
  
  
  
  
  
Table 4. Distances (cm) between the centre points of the first 
pulse mode derived buildings and map buildings. 
  
  
  
  
  
  
  
  
  
  
Flightstrip | 2L- 3L- 4L- SL- 6L- 
map map map map map 
Min dist. 7 4 6 1 6 
Max dist. 73 52 68 63 82 
Mean +Std | 25x15 | 23x14 27x14 19x15 28418 
  
  
Table 5. Distances (cm) between the centre points of the last 
pulse mode derived buildings and map buildings. 
  
Flight strip 2F-2L | 3F-3L | 4F-4L | SF-5L | 6F-6L 
  
Min dist. 1 2 | | 1 
  
Max dist. 41 51 68 35 77 
  
  
  
  
  
  
  
Mean=Std 13+10 | 17413 | 12212 | 14:9 18#16 
  
  
Table 6. Distances (cm) between the centre points of the first 
and last pulse mode derived buildings. 
Mean distances of the centre points of the extracted 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 for the first pulse and 
+14-18 em for the last pulse. Maximum distances were mainly 
less than the Toposys Falcon scan line distance, about 80 cm, in 
the across track direction. It was difficult to find the exact 
boundaries for some buildings because they were partly covered 
by trees. This is one reason for the large errors in distances 
when using the first pulse data. Distances between the centre 
points of the first and last pulse mode derived buildings 
coincide better with each other than with the map buildings. 
Mean errors (12-18 cm) and standard deviations (49-16 cm) 
from one flight strip include errors resulting from the building 
extraction modelling and from the different observation modes. 
Mean north and east differences between buildings 
from different flight strips 
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Mean differences and standard dev. 
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Compared flight strips 
Figure 2. Planimetric errors of last pulse flight strips. 3 and 5 
were flown to the southeast and 2, 4 and 6 to the 
northwest. 002-003, 004-003, 006-003, 002-005, 
004-005, 006-005 are opposite directions. 
Mean north and east differences between ridge roof 
buildings from different flight strips 
  
  
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Compared flight strips 
Figure 3. Planimetric errors of last pulse flight strips. 3 and 5 
were flown to the southeast and 2, 4 and 6 to the 
northwest. 002-003, 004-003, 006-003, 002-005, 
004-005, 006-005 are opposite directions. Only 
ridge roof buildings included. 
As mentioned in section 2.1, strips number 3 and 5 were flown 
to the southeast direction and 2, 4, 6 were flown to the 
northwest direction. We had two cases to compare. Firstly, 
flight strips to the same directions were compared and secondly, 
also the opposite direction flight strip comparisons were carried 
out, Figures 2 and 3. In Figure 3 only the ridge roof buildings 
were included because they were the biggest group and easiest 
to extract. 
In Figures 2 and 3 the first four columns (average values) on the 
left are the same flight direction pairs. Columns five to ten 
   
  
   
   
  
   
      
  
   
   
    
      
  
   
    
  
   
  
  
  
  
  
  
  
   
   
  
   
  
  
  
  
  
  
  
   
   
    
	        
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