ISPRS Commission III, Vol.34, Part 3A ,,Photogrammetric Computer Vision‘, Graz, 2002
" N : n de ë mw. qe -
Figure 10: Shading of the DTM with gross errors in the MOLA
dataset
these gross errors can be recognized. Of course, the generation
of a DTM from the whole Mars surface by manual correction is
not practicable and therefore an automatic procedure for error
elimination is required.
In the first test we tried to use hierarchical (due to the very
inhomogeneous point density) robust interpolation to eliminate
these errors. The elimination of the scan errors was possible
with this technique, but due to the roughness of the Mars
surface we also eliminated points in regions without scan errors.
The rough surface did not fit to our functional model of linear
prediction, which is able to generate very smooth surfaces.
Better results were obtained by analysing scan line segments
instead of the residuals of each individual point. It showed up
that the average filter value of a segment (i.e. RMS of the
residuals of the points belonging to this segment) could be used
to eliminate those segments with gross errors. Due to the fact
that correct scan line segments next to a segment with gross
errors also get a higher RMS it was necessary to apply this gross
error elimination in an iterative manner. Because not all points
along a scan line segment are affected by gross errors we
analysed the discrepancies of all eliminated points in respect to
a DTM computed without these gross error segments and
accepted all previous eliminated points within a certain user
defined threshold value.
This iterative method proceeds like the following:
1. Compute a DTM with all points.
2. Compute the RMS per scan line segment and eliminate lines
with a high RMS.
3. Compute a DTM with the accepted scan line segments.
4. Former eliminated points are accepted if they are within a
certain tolerance to the DTM .
5. Compute a new DTM.
A p=p(f)
20m | 75m 200m
—
f
Figure 12: Symmetric box weight function with decreasing
extend in each iteration step for the elimination of scan line
segments
0.0m
Wh 1 4 4 E *
Figure 11: Shading of the DTM after automatic gross error
elimination
The steps 2 to 5 are repeated with iteratively decreasing
tolerance values until the tolerance of the RMS per line reaches
a user defined threshold value. The results of this process can be
seen in fig. 11.
This method corresponds to the robust interpolation with a box
weight function with decreasing extend in each iteration step
(fig. 12). In contrast to the previous examples, the weight
function is not applied to the filter values of single points but
for complete scan line segments.
5. CONCLUSIONS
We have presented a very general concept of gross error
elimination for DTM generation (surface computation) and
achieved good results for the presented datasets. What can be
seen in the example section is that the general concept for gross
error elimination is the same for all projects. Only a few
parameters must be adapted to the characteristics of the specific
datasets (weight function, number of hierarchical levels). This
adaptation is performed manually. We have derived standard
parameters, which are adapted to the characteristics of each
project. This is performed in a trial and error basis with 2 or
maximal 3 repetitions of the computation. Of course only the
interpretation of the intermediate results requires human
resources, the computation itself is performed totally
automatically. In our experience most of the adaptations are
necessary in the coarse levels. The functional model for surface
computation is in the presented examples linear prediction, but
any model can be used, which is capable of considering
individual weights for the given points.
Additionally two methods of data densification have been
presented (sec. 4.1 and 4.3).
In the future we will have to consider new measurement
systems, which will provide further information of the sensed
objects like laser scanner systems, which allow now the
registration of multiple echoes and the intensities of the
returned signal and in future even full waveform capture. An
other important topic will be sensor combination. Nowadays
sensor systems, which combine laser scanner sensors with
digital line cameras, already do exist. The big task for the future
will be to integrate all these information sources into one
modelling process in order to achieve better results.