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ASSESSMENT OF DEM ACCURACY DERIVED FROM SPOT-5 HIGH RESOLUTION
STEREOSCOPIC IMAGERY
W. Kornus, R. Alamüs, A. Ruiz, J. Talaya
Institut Cartografic de Catalunya (ICC), Parc de Montjuic, E-08038 Barcelona
wkornus@ice.es, ralamus@icc.cs, toni@ice.es, talaya@icc.es
Commission I, WG 1/2
KEY WORDS: SPOT, Space Photogrammetry, Orientation, Adjustment, DSM/DTM, Comparison, Accuracy
ABSTRACT:
This paper describes the derivation of Digital Surface Models (DSMs) from 3-fold along-track stereoscopic SPOT-5 imagery in the
scope of the HRS (High Resolution Stereoscopic) study, organized by the Centre Nacional d'Études Spatiales (CNES) and the
International Society of Photogrammetry and Remote Sensing (ISPRS). The orientation of SPOT-5 is reconstructed by bundle
adjustment using a functional model based on correction polynomials. It resulted in an RMS-error of 2 m in Easting, Northing and
Height at 17 check points. DSMs are produced for 4 test sites, which are located in different terrain types (mountainous, moderate and
urban). An automatic region growing image matching process generates a dense point cloud in image space, which later is rigorously
transformed into the object space and converted into a regular spaced DSM. The comparison with a digital terrain model (DTM) of
superior accuracy yields standard deviations better than 5 m (16) in flat and moderate terrain and better than 10 m (16) in mountainous
regions. An additional DSM covering the entire image scene (approx. 60 km x 80 km) is produced with a standard deviation of
approximately 8 m using the commercial software ISAE and rational functions. The sigma values include all errors of the automatic
matching process as well as the differences between the surface and the terrain model and therefore must be regarded as conservative.
All results are finally summarized and conclusions are drawn from the study.
1. THE SPOT-5 SATELLITE
SPOT-5 is the first satellite of the SPOT family with along-
track stereo imaging capability. The two HRS cameras are
tilted by +/- 20 degrees and acquire nearly simultaneous
stereopairs (at a 90-second interval) of 120 km swath, along
the track of the satellite, with a B/H ratio of 0.84. A
continuous strip of 600 km length is covered stereoscopically
with 10 m ground sampling distance (GSD) across track and
with 5 m GSD along track. The nadir looking panchromatic
HRG instrument provides imagery in the mono-spectral
bands HMA and HMB at 5 m GSD, in the multi-spectral
bands XS1, XS2, XS3 at 10 m and SWIR at 20 m GSD. The
ground pixels of HMA and HMB scenes are interleaved to
enable the interpolation of so-called THR ‘supermode’
images(SPOT Magazine, 2000), having a nominal GSD of
2.5m. A summary of the SPOT-5 payload and mission
characteristics is given in (Fratter et al., 2001). The size of an
image scene is 12000 x 12000 pixel (24000 x 24000 pixel in
case of the THR ‘supermode’ image).
2. INITIAL DATA
The study was conducted using an image scene covering
Barcelona and the surrounding area. The data set provided by
CNES comprised 5 images (HRS1, HRS2, HMA, HMB and
the THR supermode image) and auxiliary data (time series of
orbit positions, velocities and attitude angles, look angles for
each CCD element, etc.). The ICC provided the reference
data set consisting of a regular DTM of 15 m grid size and
1.1 m accuracy (1 opqy) covering the total area of the images
and of 32 orthoimages of 0.5 m pixel size and 0.5 m accuracy
(16) for 8 well distributed, approximately 10 x 14 km wide
test sites (TS) (see figure 1). Figure 2 shows the two
radiometrically improved and strongly reduced images of the
THR and the HRS1 channels. The different resolutions of the
HRSI image in scan and flight direction are clearly visible.
aae dd
mun
Figure 1: Location
i P2 1 P í 3
es aie i v bo edi ejl it V I
ISI AN EE E
of
the
reference DTM
rectangle) and the 8 test sites
Figure 2: THR image (left, GSD: 2.5m x
(d
image (right, GSD: 10m x 5m)
(light blue
2.5m) and HRSI