Full text: Proceedings; XXI International Congress for Photogrammetry and Remote Sensing (Part B4-3)

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The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences. Vol. XXXVII. Part B4. Beijing 2008 
is completed with field data to obtain cartography of urban 
areas, the digitization of more objects during the stereoplotting 
could reduce field data capture. Unfortunately no analysis has 
yet been done to know in detail the impact of this reduction, 
although that the estimated percentage will not achieve in any 
case more than 4 or 5%. In small scale flights it has not been 
possible to extend the flight period because the requirements in 
radiometry for orthophoto products require flights taken from 
May to September. 
The second advantage is that usually the sharpness of the DMC 
images is higher than the obtained in the analogical ones at any 
scale, so the vector digitization is more comfortable for the 
operators. 
The main disadvantage is a slight loss of the relief feeling. In 
large scale digital flights, with 7.5cm GSD, it is quite difficult 
to measure the height in objects lower than 20cm, like sidewalk 
curbstones or the rails of railways. These short measurements in 
height were possible using images taken by analogical cameras. 
This slight imprecision in the component H introduces some 
insecurity and uncomfortable feeling during the stereoplotting 
process. 
Another disadvantage is the big differences in contrast between 
dark and bright areas. If the photogrammetric system doesn’t 
include some tools to modify more or less automatically the 
histogram during the stereoplotting process, the digitization 
process is harder than in the case of using analogical images 
where the contrast was not so high. 
The last disadvantage is related to the reduction of the area 
covered by the digital stereopairs. It implies to manage twice as 
much files than in the case of analogical stereopairs and 
represents an extra cost during the stereoplotting process if the 
system hasn’t tools to change automatically to the adjacent 
stereopair. 
6. IMAGE RESOLUTION 
Traditionally, the resolving power of an optical system was 
measured by the visual identification of targets, amongst which 
the USAF 1951 test stood out due to the fact that it has been 
used more than others. With the same purpose electronic 
methods have been developed to assess the performance of a 
system, based on profiles of sinusoidal intensity and supported 
by the Modulation Transfer Function (MTF) and the Edge 
Spread Function (ESF). Our methodology is based on the latter. 
A software tool is implemented with the aim of providing a 
resolving measurement of an image in pixel magnitude. The 
program processes a region of interest that contains a single 
contour and makes a minimum square adjustment over the bi- 
dimensional function of the edge that we model as a sigmoid 
function: 
f(j’i) P4 J -P 3 (/-cos P 5 +ysin P 5 -P 2 ) W 
P k e%k = 1,...,5. 
The five parameters are estimated in a least squares adjustment 
and the computed function is derived for obtaining the LSF 
(Line Spread Function). We consider the FWHM (Full Width at 
Half Maximum) over the LSF to be the measurement value. 
6.1 Results obtained with aerial images (DMC) and 
Siemens star targets 
The algorithm has been applied on a Siemens star target painted 
on a canvas surface of 100m 2 that has been captured in four 
DMC aerial images. The pattern used for this study can be seen 
on the top-right part of Figure 5. On each of the four images 
used for the test, the pattern was located at a different distance 
from the centre. The average resolution obtained for each image 
is shown in table 9. 
Figure 5: Siemens star target used for the resolution study 
Image 
Distance 
to the 
centre 
(pixel) 
Resolution 
(pixel) 
Image 1 
1772 
0.83 
Image 2 
1519 
0.79 
Image 3 
4241 
1.07 
Image 4 
4543 
1.32 
Table 9: Resolution measurements as function of the distance 
from the image centre 
These results show that the distance to the centre of the image 
greatly affects the resolution. The main reason that explains this 
behaviour is the formation of the large format image from 
oblique component images. The 12pm size pixel gives us a 
nominal resolution of 84 1/mm. But, in fact, the resolution is not 
constant in the whole area of the large format virtual image. 
The sensor is tilted along the two axis x and y. This factor has 
been studied by Honkavaara et al. 2006 who obtained a 
resolution of 53 and 84 1/mm perpendicular to the direction of 
flight and around 60 and 84 1/mm in the direction of flight. 
6.2 Results obtained with aerial images (DMC) on urban 
settings. 
Finally, the aim is to apply concepts and techniques developed 
to images captured with DMC that do not have, necessarily, 
artificial models. Due to their radiometric and morphological 
characteristics (close to the USAF model) we chose to apply the 
software on images of urban settings. Adequate radiometric 
contours are considered to be road markings and, more 
precisely, pedestrian crossings, see Figure 6.
	        
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