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In this chapter we extend the works of Piper and Granum
[122] and Verwer et al. [167] on geodesic
distances. First, we generalize the definition of geodesic
distances. Secondly, we propose two algorithms to compute the new
geodesic DT. Thirdly we evaluate how accurately these algorithms
approximate the Euclidean metric. Finally, we study their
computational complexity.
Olivier Cuisenaire
1999-10-05