Full text: XVIIIth Congress (Part B4)

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back-packed design makes single man surveying feasible 
and it is ideally suited to the collection of 
photogrammetric control points. Using post-processed 
differential correction, Trimble claim the corrected C/A 
code provides an accuracy of ‘better than one metre’ on a 
second-by-second basis. There are however several 
degrading factors to this, such as the distance to the 
base station and the number of satellites available. The 
survey was carefully planned to avoid times of poor 
satellite configuration and the Surveying Department's 
SciNet pillar was used as a base station in the centre of 
the survey area so keeping the distance between base 
and rover below 1 km. The main degrading factor (other 
than selective availability) of the survey in this case was 
found to be that of multipathing - a problem that is very 
difficult to overcome in a city centre site when using only 
C/A code differential processing. In an attempt to 
surmount this problem, each control point was observed 
with the antenna mounted on a bipod for a period of five 
minutes so as to provide an averaged position. 
The points were differentially post-processed and 
converted from WGS84 to OSGB36 using a four 
parameter local transformation. ^ This allowed the 
referencing of the imagery to the OS data of the area. A 
check on a point of known co-ordinates at the periphery 
of the survey area showed this method of GPS 
observation to give average errors of 0.84 m in plan and 
1.25 m in height. Unfortunately this is larger than the 
ground pixel size, although the collection of some 60 
control points allowed rejection of any inaccurately co- 
ordinated points. The two images being used for the 
survey were orientated and rectified using the GCPs. 
The space resection performed to orientate the imagery 
yielded the orientation parameters shown in Table 1. It 
can be seen from the GCP residuals that the RMS error 
is at the sub-pixel level. 
  
  
  
  
  
  
  
  
  
  
  
  
  
  
Image 81 Image 82 
X (m) 424784.37 424634.54 
Y (m) 565100.22 564858.91 
Z (m) 1494.56 1494.43 
degrees) -4.160 -2.993 
degrees) 3.305 0.689 
K (degrees) 151.605 151.149 
Datum height (m) 58.46 64.28 
Base/Height ratio 0.19 
No. of GCPs 36 43 
RMSE (pixels) 0.96 0.86 
RMSE (m) 0.44 0.39 
  
  
posterizing effect and setting the measuring mark can 
prove difficult in areas of low contrast. 
The stereopair was then autocorrelated to produce a 
Digital Elevation Model (DEM) of the area. This enabled 
the imagery to be geometrically corrected for relief 
displacement to create an orthophoto. The area based 
matching technique employed by the DMS is suited 
ideally to gently undulating areas and inevitably the 
disjointed nature of a city centre site causes many 
failures in correlation, leading to lengthy editing times. 
Every pixel in the image was correlated and rectified in 
an attempt to correct the buildings for lean. There is 
considerable masking of ground detail due to building 
lean on the imagery, and a facility to recover this from 
adjacent images, such as the technique employed by the 
Leica Helava system (Simmons, 1996) would be useful in 
such circumstances. Measurements on the orthophoto of 
the same GPS control points used in the stereo tests 
produced RMS errors of 0.94 m (2.1 pixels) in plan and 
1.71 m (3.8 pixels) in height. 
3.4 Mapping Accuracy 
Measurements taken against the GCPs are unlikely to 
give a true representation of the absolute accuracy of the 
survey since they have been used in orientating the 
imagery. To ascertain the absolute accuracy of co- 
ordinates produced from the images, a total of 70 
randomly chosen points were measured from the OS 
digital mapping of the area. This data has a quoted RMS 
error of 0.4 m (Ordnance Survey, 1995). The same 
points were then measured on the stereomodel and the 
orthophoto (with heights from the DEM). The results of 
the comparison can be seen in Table 2. Unfortunately 
the table shows no measure of heighting accuracy or 
precision since the OS dataset is two dimensional. The 
stereomodel and orthophoto measurements were 
therefore compared, yielding an RMS error in height 
between the two of 0.90 m (2 pixels). Precision (obtained 
by 10 repeated measurements to 6 different points) for 
the heighting was calculated as 0.39 m (0.9 pixels) RMS 
error for the stereo measurement. Orthophoto height 
measurements showed almost perfect repeatability, 
although this can be attributed to the resolution of the 
DEM. 
  
  
  
  
  
  
Table 1: Orientation parameters and GCP residuals of 
the imagery used in the Newcastle survey. 
3.3 Photogrammetric Processing 
Stereoscopic tests on the 15 GCPs on the overlap 
produced RMS errors of 1.02 m (2.3 pixels) in plan and 
1.79 m (4.0 pixels) in height. The accuracy to which one 
Can measure is, however, degraded by the DMS’s 
anaglyph stereoviewing facility. Despite the fact that the 
monitor can display 32,000 colours, the display driver 
only supports 8 bit colour with each of the images 
displayed using four bits (16 grey levels) to represent the 
296 levels recorded by the camera. This gives a 
565 
  
  
  
  
  
  
  
  
  
  
Accuracy 
Method X RMSE Y RMSE 
Metres Pixels Metres Pixels 
Stereo 0.79 1.8 0.55 1.2 
Ortho 0.52 1.2 0.48 1.1 
Repeatability (Precision) 
Method X RMSE Y RMSE 
Metres Pixels Metres Pixels 
Stereo 0.09 0.2 0.10 0.2 
Ortho 0.10 0.2 0.09 0.2 
  
  
  
Table 2: Accuracy and repeatability statistics for the 
Newcastle survey (comparison against OS). 
As a check, the GPS control was also compared to the 
OS data, resulting in an RMS error of 0.84 m in the east- 
west (x) direction and 1.16 m in the north-south (y) 
direction. 
International Archives of Photogrammetry and Remote Sensing. Vol. XXXI, Part B4. Vienna 1996 
 
	        
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