International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Vol XXXV, Part B1. Istanbul 2004
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relative L track (meters) relative L track (meters)
Before modification After modification
Figure 4 : improvement of HRS relative location
(ellipse is the 3 x std boundary)
As for HRS absolute location performance, the analysis showed
an important variation of the performance depending with the
latitude of the acquisition. This variation was firstly thought to
be related to a specific thermoelastic effect affecting the whole
payload as it,also touched HRG's location performance. The
explanation of this variation finally appeared to be a bad
initialisation of the star tracker relativist compensation process.
After on board correction of this problem, no more variation of
the performance with latitude has been observed and HRS
absolute system location performance without using any ground
model went down from 50 m rms to 20 m rms (see figure 5).
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absolute L track (meters) absolute L track (meters)
Before modification After modification
Figure 5 : improvement of HRS absolute location
(ellipse is the 3 x std boundary)
An analytic model has been calibrated in order to improve on
ground the location performance before the modification (see
[Bouillon, 2003]). This model is not to use for images acquired
after the modification. Moreover, it should be replaced by a
rigorous description of the effect as known for a correct
description of the impact on images acquired before the
modification.
Finally, taking into account all this knowledge, the analysis of
remaining location errors for all images shows a temporal trend,
combination of ageing, seasonal stability and discontinuity due
to the on board modification of HRS' foot thermal control (see
figure 6). This trend can be modelled and taken into account on
ground for further improvement of the location performance.
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Pitch (microrads) Roll (microrads)
Yaw (microrads)
Figure 6 : Satellite Roll, Pitch and Yaw temporal trend
computed out of HRS' absolute location performance
3.3 Stereoscopic and Reference3D performances analysis
Analysis of the horizontal accuracy of HRS stercopairs, and
blocks of HRS strips (Reference3D performances) have been
assessed in collaboration with French National Geographic
Institute. Main results are presented in [Airault, 2003] and
[Airault, 2004].
First of all, the processing of HRS blocks takes into account a
specific model for images acquired before removal of the on
board relativist error, and a temporal model for all images
including remaining effects described above. These are
necessary to obtain the best location performance possible for
all available images.
Remaining errors are measured through bundle block
adjustment by taking into account tie points between two
images of an HRS stereopair, and between different HRS strips.
The analysis of the process showed out that considering HRS
instrument as rigid was a necessary hypothesis to manage it. It
is therefore admitted that HRS' internal parameters do not vary
with time : this reduces the degrees of freedom and allows a
good solution.
Moreover, some possible improvement of HRS inner
orientation parameters were pointed out. In particular, among
Reference3D production, a 3000 km wide block is available
which allows a very precise measure of camera's focal length.
Finally, this work was carried out on every location site
available, and also on some Reference3D production sites (total
of more than 20 sites all over the world). It showed out that
availability of precise ground control points is the key for a
good interpretation of errors. As a matter of fact, priority was
given to sites with GPS points in order to get rid of some
possible biases of local cartographic systems.
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