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The key to three-view geometry

机译:三视图几何的关键

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In this article we describe a set of canonical transformations of the image spaces that make the description of three-view geometry very simple. The transformations depend on the three-view geometry and the canonically transformed trifocal tensor T' takes the form of a sparse array where 17 elements in well-defined positions are zero, it has a linear relation to the camera matrices and to two of the fundamental matrices, a third order relation to the third fundamental matrix, a second order relation to the other two trifocal tensors, and first order relations to the 10 three-view all-point matching constraints. In this canonical form, it is also simple to determine if the corresponding camera configuration is degenerate or co-linear. An important property of the three canonical transformations of the images spaces is that they are in SO(3). The 9 parameters needed to determine these transformations and the 9 parameters that determine the elements of T' together provide a minimal parameterization of the tensor. It does not have problems with multiple maps or multiple solutions that other parameterizations have, and is therefore simple to use. It also provides an implicit representation of the trifocal internal constraints: the sparse canonical representation of the trifocal tensor can be determined if and only if it is consistent with its internal constraints. In the non-ideal case, the canonical transformation can be determined by solving a minimization problem and a simple algorithm for determining the solution is provided. This allows us to extend the standard linear method for estimation of the trifocal tensor to include a constraint enforcement as a final step, similar to the constraint enforcement of the fundamental matrix. Experimental evaluation of this extended linear estimation method shows that it significantly reduces the geometric error of the resulting tensor, but on average the algebraic estimation method is even better. For a small percentage of cases, however, the extended linear method gives a smaller geometric error, implying that it can be used as a complement to the algebraic method for these cases.
机译:在本文中,我们描述了一组图像空间的规范转换,这些描述使三视图几何的描述非常简单。变换取决于三视图几何,并且经规范变换的三焦点张量T'采用稀疏数组的形式,其中在明确定义的位置中的17个元素为零,它与摄影机矩阵和两个基本矩阵具有线性关系矩阵,与第三基本矩阵的三阶关系,与其他两个三焦点张量的二阶关系以及与10个三视图全点匹配约束的一阶关系。以这种规范形式,也很容易确定相应的摄像机配置是简并的还是共线性的。图像空间的三个规范变换的一个重要属性是它们在SO(3)中。确定这些变换所需的9个参数和确定T'的元素的9个参数一起提供了张量的最小化参数。它不存在其他参数化所具有的多个映射或多个解决方案的问题,因此易于使用。它还提供了三焦点内部约束的隐式表示:当且仅当三焦点张量与其内部约束一致时,才能确定三焦点张量的稀疏规范表示。在非理想情况下,可以通过解决最小化问题来确定规范变换,并提供用于确定解的简单算法。这使我们能够扩展用于估计三焦点张量的标准线性方法,使其包括约束执行作为最后一步,类似于基本矩阵的约束执行。对这种扩展线性估计方法的实验评估表明,它可以显着降低所得张量的几何误差,但平均而言,代数估计方法更好。但是,在少数情况下,扩展线性方法的几何误差较小,这意味着可以将它们用作这些情况的代数方法的补充。

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