ation estimate
edicted |
del 2 = ^
LZ.
50 180
©
30 60 90 120 150 180
Time, s
Figure 7. Recovered orientation angle 9
28 — —3
2% C ! l sareassesestutass; model
30 60 90 120 150 180
Time, s
Figure 8. Recovered orientation angle x
The algorithm allows tracking objects given their 3D models.
The convergence of the iterative algorithm depends on the
availability of a good initial estimate. The procedure of
recovering orientation parameters is ambiguous since there are
many configurations that give rise to approximately the same
projected contours. It may happen that the algorithm does not
converge to the right optimum; this is due to the presence of
false edges such as structures that are parallel to the true edges.
Contours of the docking module should allow resolving the
ambiguities in the determination of angles — however, since the
docking module is small relative to the ISS a whole, the
contribution of its contours in the whole misfit function is
relatively modes. False edges often arise from shadows,
especially long and contrasting shadows are cast by solar
panels. In some flybys, additional distracting contours appear
due to the texture of the Earth’s atmosphere.
Then the algorithm was tested on a real video with only visual
quality assessment. The real dataset contained telemetry
information which was overprinted on the video sequence.
Pixels belonging to textual information have been ignored by
means of a binary mask which was created offline. Along with
high noise level, flare and unfavorable lighting conditions it
makes the problem of ISS image matching very difficult (Figure
9). The total fraction of successful image matching for real
video frames is 20-30% less then in case of modelling video.
An example of successful fitting of the contour template to the
real video frame is shown in Figures 10 and 11.
CERTA EE
EAE EDT ES]
Figure 11. Contour obtained from found orientation
4. CONCLUSION
In this work we presented a method for estimating the
orientation parameters based on the use of a highly detailed
digital model of the ISS. One of specific features of the problem
that we studied is that the ISS appearance on video frames
substantially changes in the course of docking approach.
Analysis shows that solving such a recognition and tracking
problem requires different sets of algorithms depending on the
range of distances between the SCS and ISS.
In order to solve the exterior orientation problem for frame
image of ISS the contour-based algorithms are used. Statistical
tools such as Kalman filter are used to support the estimation
process and real time object tracking. The substantial feature of
the method presented in this work is the usage of a very detailed
digital 3D model of ISS for subsequent generation of raster
wireframe templates, used for detection in each frame and
tracking of the ISS in video sequence. Algorithms based on the
usage of wireframe templates show high robustness, but