ESSEN
Fig.2: Test a
A A
k: k
1.0 LCD cos i 1.0 (1-s)*s cos'e
x. ;
cos'e >. : |
»
So At AAT A,
Fig. 1: Extended normalisation funktion
As already mentioned above the correction due to the
observation angle will not be pursued any longer in our
current work. We recommend further investigations. The
examples later show that the influence of the observation
angle seems to be negligibly small.
Before we continue with the determination of the para-
meters of the normalisation function it is advisible to prove
that in reality this function may serve as suitable model. For
that reason we chose our test area in the Austrian Alps
where high mountains and steep slopes guarantee all sorts
of illumination effects, from brightly sun lit regions with
incidence angles around 0°, to dark shadows where the
(virtual) incidence angle is greater than 90°, all sorts of
shades in between, and eventually even cast shadows.
Figure 2 shows an overview of the some 35 km x 25 km
large area in the so-called "Salzkammergut" with its lakes.
We use in our investigation the six optical bands of a
Landsat TM image (1 to 5 and 7).
The DTM provided by the Austrian Federal Office for
Metrology and Surveying has a grid width of 25 m x 25 m.
The geometrically rectified satellite image has the same
ET EEE NC CUP NUDO SORS asc
rea located in the Austrian Salzkammergut (Landsat TM, Band 4)
resolution. We want to emphasize that the geometric
rectification must be performed with the help of a parametric
model, so that displacements due to terrain heights are also
rectified. In our case we used the bundle block adjustment
program ORIENT [Kager, 1989] in conjunction with the
digital orthophoto modul of SCOP DOP [Molnar et al. 1998].
High geometric accuracy is a prerequisite for a good quality
of topographic normalisation in particular along terrain
discontinuities, such as steep ridges or narrow valleys.
Fig.3: cos i of the DTM (black = i greater 90°)
10 Intemational Archives of Photogrammetry and Remote Sensing. Vol. XXXII, Part 7, Budapest, 1998
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