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this chapter, four crater-detection methods have been presented and discussed with
various extent of discrimination ability on planetary images or topography data. The
modified Adaboosting approach demonstrates the best performance in classification
of craters. The algorithms which are based on topography data are of low efficiency
in automatic detection. However, considering that topography data can provide 3D
structure of craters, it is necessary to develop new algorithms to improve efficiency.
In the future, more work should be done to investigate the possibility of using a
hybrid method by combining optical images with topography data.
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