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Space curves are one-parameter manifolds immersed in Euclidean 3D space \(\mathbf{r}(s) \subset {\mathbb{E}}^{3}\), where \(s \in \mathbb{R}\). One requires differentiability to whatever order is necessary, and \(\|{\frac{\partial \mathbf{r}(s)} {\partial s} \|}^{2}\neq 0\). It is convenient to require \(\|{\frac{\partial \mathbf{r}(s)} {\partial s} \|}^{2} = 1\), though this can always be achieved through a reparameterization. Such curves are known as “rectified” or “parameterized by arc-length,” and one writes \(\mathop{\mathbf{r}}\limits^{.}(s)\) for the partial derivative with respect to arc-length (r′(t) will be used if the parameter t is not arc-length). As discussed below, in addition one requires \(\mathop{\mathbf{r}}\limits^{..}(s)\neq 0\)for a generic space curve. The very notion of “rectifiable” is of course Euclidean. Curves in...
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Koenderink, J.J. (2014). Curves in Euclidean Three-Space. In: Ikeuchi, K. (eds) Computer Vision. Springer, Boston, MA. https://doi.org/10.1007/978-0-387-31439-6_644
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DOI: https://doi.org/10.1007/978-0-387-31439-6_644
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