TY - JOUR
T1 - Robust depth estimation for light field via spinning parallelogram operator
AU - Zhang, Shuo
AU - Sheng, Hao
AU - Li, Chao
AU - Zhang, Jun
AU - Xiong, Zhang
N1 - Publisher Copyright:
© 2016 Elsevier Inc. All rights reserved.
PY - 2016/4
Y1 - 2016/4
N2 - Removing the influence of occlusion on the depth estimation for light field images has always been a difficult problem, especially for highly noisy and aliased images captured by plenoptic cameras. In this paper, a spinning parallelogram operator (SPO) is integrated into a depth estimation framework to solve these problems. Utilizing the regions divided by the operator in an Epipolar Plane Image (EPI), the lines that indicate depth information are located by maximizing the distribution distances of the regions. Unlike traditional multi-view stereo matching methods, the distance measure is able to keep the correct depth information even if they are occluded or noisy. We further choose the relative reliable information among the rich structures in the light field to reduce the influences of occlusion and ambiguity. The discrete labeling problem is then solved by a filter-based algorithm to fast approximate the optimal solution. The major advantage of the proposed method is that it is insensitive to occlusion, noise, and aliasing, and has no requirement for depth range and angular resolution. It therefore can be used in various light field images, especially in plenoptic camera images. Experimental results demonstrate that the proposed method outperforms state-of-the-art depth estimation methods on light field images, including both real world images and synthetic images, especially near occlusion boundaries.
AB - Removing the influence of occlusion on the depth estimation for light field images has always been a difficult problem, especially for highly noisy and aliased images captured by plenoptic cameras. In this paper, a spinning parallelogram operator (SPO) is integrated into a depth estimation framework to solve these problems. Utilizing the regions divided by the operator in an Epipolar Plane Image (EPI), the lines that indicate depth information are located by maximizing the distribution distances of the regions. Unlike traditional multi-view stereo matching methods, the distance measure is able to keep the correct depth information even if they are occluded or noisy. We further choose the relative reliable information among the rich structures in the light field to reduce the influences of occlusion and ambiguity. The discrete labeling problem is then solved by a filter-based algorithm to fast approximate the optimal solution. The major advantage of the proposed method is that it is insensitive to occlusion, noise, and aliasing, and has no requirement for depth range and angular resolution. It therefore can be used in various light field images, especially in plenoptic camera images. Experimental results demonstrate that the proposed method outperforms state-of-the-art depth estimation methods on light field images, including both real world images and synthetic images, especially near occlusion boundaries.
KW - Depth estimation
KW - Epipolar plane image
KW - Light field
KW - Spinning parallelogram operator
UR - https://www.scopus.com/pages/publications/84961216956
U2 - 10.1016/j.cviu.2015.12.007
DO - 10.1016/j.cviu.2015.12.007
M3 - 文章
AN - SCOPUS:84961216956
SN - 1077-3142
VL - 145
SP - 148
EP - 159
JO - Computer Vision and Image Understanding
JF - Computer Vision and Image Understanding
ER -