A closed form self calibration of one-dimensional light stripe feature width function for indoor navigation

H. Jung, J. Suhr, Hyoung-Jin Kang, Jaihie Kim
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引用次数: 5

Abstract

Light stripe projection (LSP) is one of useful methods to recognize 3D information in various vision applications. In general, light stripe feature (LSF) is detected by LOG (Laplacian Of Gaussian) operator. Because LOG variance parameter is corresponding to LSF width, improper parameter value causes severe performance degradation. Our previous work proposed a method predicting LSF width by modeling LSF irradiance as 2D Gaussian function [1]. Although the method could enhance the performance of LSF detection, calibration method included time consuming genetic algorithm-based optimization procedure. This paper proposes a closed form calibration method assuming LSF irradiance can be approximated as 1D Gaussian function if field of view (FOV) of light plane projector (LPP) is much wider than that of camera or the LPP generates uniform LSF. Experimental results show that derived function can correctly predict LSF width, and related parameters can be calibrated in a closed form.
一种用于室内导航的一维光条特征宽度函数的封闭自标定方法
在各种视觉应用中,光条投影(LSP)是识别三维信息的有效方法之一。一般来说,光条特征(LSF)是通过LOG (laplace Of Gaussian)算子来检测的。由于LOG方差参数对应LSF宽度,参数取值不当会导致严重的性能下降。我们之前的工作提出了一种通过将LSF辐照度建模为二维高斯函数来预测LSF宽度的方法[1]。虽然该方法可以提高LSF检测的性能,但标定方法包含耗时的遗传算法优化过程。本文提出了一种闭式定标方法,假设光平面投影仪(LPP)的视场(FOV)比相机宽得多,或者LPP产生均匀的LSF时,LSF辐照度可以近似为一维高斯函数。实验结果表明,导出的函数可以正确地预测LSF宽度,并且可以以封闭的形式校准相关参数。
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