cvpr cvpr2013 cvpr2013-147 knowledge-graph by maker-knowledge-mining

147 cvpr-2013-Ensemble Learning for Confidence Measures in Stereo Vision


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Author: Ralf Haeusler, Rahul Nair, Daniel Kondermann

Abstract: With the aim to improve accuracy of stereo confidence measures, we apply the random decision forest framework to a large set of diverse stereo confidence measures. Learning and testing sets were drawnfrom the recently introduced KITTI dataset, which currently poses higher challenges to stereo solvers than other benchmarks with ground truth for stereo evaluation. We experiment with semi global matching stereo (SGM) and a census dataterm, which is the best performing realtime capable stereo method known to date. On KITTI images, SGM still produces a significant amount of error. We obtain consistently improved area under curve values of sparsification measures in comparison to best performing single stereo confidence measures where numbers of stereo errors are large. More specifically, our method performs best in all but one out of 194 frames of the KITTI dataset.

Reference: text


Summary: the most important sentenses genereted by tfidf model

sentIndex sentText sentNum sentScore

1 nz Abstract With the aim to improve accuracy of stereo confidence measures, we apply the random decision forest framework to a large set of diverse stereo confidence measures. [sent-4, score-1.766]

2 Learning and testing sets were drawnfrom the recently introduced KITTI dataset, which currently poses higher challenges to stereo solvers than other benchmarks with ground truth for stereo evaluation. [sent-5, score-0.99]

3 We experiment with semi global matching stereo (SGM) and a census dataterm, which is the best performing realtime capable stereo method known to date. [sent-6, score-1.176]

4 We obtain consistently improved area under curve values of sparsification measures in comparison to best performing single stereo confidence measures where numbers of stereo errors are large. [sent-8, score-1.756]

5 Introduction A vast amount of algorithms to solve the stereo problem have been proposed with the target to yield improved error statistics on popular benchmarking datasets. [sent-11, score-0.518]

6 Recently, this issue has been approached through definition of a more challenging benchmark [9], and further improvements on performance of stereo solvers are anticipated. [sent-13, score-0.447]

7 We illustrate this for the stereo case: If, in a worst case scenario, one of the two cameras fails, dense matching results can be computed, but these are not reliable in any location. [sent-16, score-0.536]

8 de quite effective, by plotting consistency gaps over disparity errors, see Figure 1. [sent-22, score-0.418]

9 Applications where accurate stereo confidence measures are essential in raising reliability of computer vision include sparse [19] or dense [16] 3D scene reconstructions. [sent-23, score-0.95]

10 This has initiated attempts to combine several confidence measures with the aim of achieving superior accuracy in detection of bad matching estimates. [sent-26, score-0.661]

11 Previous solutions [14, 17] were based on a very limited set of features capturing confidence and were tested only on data not presenting much challenge to stereo. [sent-27, score-0.365]

12 In this paper, we employ strong energy based confidence clues and use a larger and significantly more challenging stereo dataset introduced recently [9], where results compare much better to real-world scenarios than was the case with benchmarks proposed previously. [sent-28, score-0.88]

13 Section 3 details challenges in defining confidence for matching tasks, compiles some proposals for stereo confidence definition and introduces new confidence definitions used in this paper. [sent-30, score-1.718]

14 Section 4 explains the machine learning framework used for confidence accuracy improvements. [sent-31, score-0.365]

15 Related Work Kong and Tao [14] proposed a stereo matcher, where distributions of labels for good, bad and foreground fattening affected disparities are estimated in a MAP-MRF framework based on horizontal texture and distances to closest foreground objects drawn from ground truth. [sent-36, score-0.654]

16 [17] derived binary confidence labels by learning from a larger set of features amenable to hardware processing using decision trees and ANNs. [sent-38, score-0.461]

17 Error of SGM stereo result to ground truth plotted against left-right difference of corresponding points in disparity maps of both views. [sent-40, score-0.89]

18 For optical flow, Gehrig and Scharw¨ achter [8] used Gaussian mixtures to model a feature space composed of spatial and temporal flow variance, residual flow energy and structure tensor eigenvalues on small image patches. [sent-44, score-0.231]

19 Multi-cue confidence was defined as classification outcome according to the highest class posterior. [sent-46, score-0.365]

20 This is expressed in the idea that a confidence measure can successfully select best fitting results from multiple algorithms, ignoring the fact that flow is often undefined, e. [sent-56, score-0.482]

21 Regarding above mentioned confidence features for opti- cal flow [2], image gradients in conjunction with flow variance are likely to detect lowly textured areas in input images with high variance in flow. [sent-60, score-0.722]

22 However, in stereo and motion alike, reasons for failure may not be restricted to low texturedness. [sent-62, score-0.487]

23 Hence, using a more diversified set of confidence measures as contributing features is very likely to result in improved accuracy for good or bad pixel detection due to consideration for an increased number of possible reasons for algorithm failure. [sent-63, score-0.676]

24 So, in the following section, we discuss various stereo confidence measures proposed in the literature, and attempt to motivate a selection of most promising measures. [sent-64, score-0.978]

25 Confidence Measures for Stereo Causes for errors in disparity estimation within a global stereo optimization framework can be based on inappropriate model assumptions, highly nonconvex energies causing multiple strong local minima or numerically instable global minima. [sent-66, score-0.915]

26 Assuming error prediction worked out, we would know error magnitudes and could plug these into the stereo estimation model to improve stereo results directly. [sent-68, score-1.069]

27 However, we can only hope to gain knowlege about suitability of signals to provide good estimates of stereo disparities in most cases, e. [sent-69, score-0.534]

28 In the absense of a strong theoretical foundation to account for properties of global energies in commonplace stereo aggregation schemes, many spatially local stereo confidence measures have been proposed [5, 13]. [sent-73, score-1.443]

29 However, evaluation has been carried out for a local stereo matching algorithm and on a small dataset only. [sent-74, score-0.536]

30 Below we briefly discuss the most prominent proposals for stereo confidence. [sent-76, score-0.493]

31 To clarify the intention behind defining confidence measures for matching, we would like to point out again, that confidence is not supposed to be a measure for potential disparity error magnitudes. [sent-77, score-1.411]

32 For low confidence matching situations, no improved or specialist algorithm may exist for obtaining a solution. [sent-80, score-0.454]

33 Good confidence measures detect areas that cannot be matched reliably. [sent-81, score-0.55]

34 333000666 In the following definitions, c refers to matching costs resulting from a Semi global matching (SGM) [11] aggregation scheme. [sent-82, score-0.315]

35 Curvature of a parabola fit to matching costs c for subpixel estimation at a pixel p is frequently considered to be a confidence measure. [sent-83, score-0.545]

36 The peak ratio measure is widely used in descriptor matching to reject correspondences with close matching costs which are believed to be ambiguous. [sent-86, score-0.447]

37 In the following, d1 denominates the disparity with lowest associated cost c(p, d1) and d2 is a disparity where c(p, d2) is a local minimum with second lowest cost at pixel p. [sent-87, score-0.894]

38 The peak ratio for a disparity at pixel p is then defined as Γ0(p) = c(p, d1)/c(p, d2) . [sent-88, score-0.553]

39 i Entropy somf disparity costs for controlling a diffusion process in cost aggregation [20] attracted some attention as a potential confidence measure. [sent-93, score-0.949]

40 1, consistency between left and right disparity is an established criterion for identification of mismatches and occlusions [11]. [sent-108, score-0.453]

41 The definition requires disparity maps Dl and Dr of left and right image: Γ3(p) = ? [sent-109, score-0.418]

42 This motivates the definition of horizontal gradient as a confidence measure: Γ4(p) =? [sent-119, score-0.402]

43 However, Γ5 may be less suitable if used in conjunction with stereo algorithms that frequently locate discontinuities well. [sent-125, score-0.508]

44 This may be the case in segmentation based stereo approaches. [sent-126, score-0.447]

45 A measure coined disparity ambiguity here is introduced to capture potential error magnitudes for the case of mismatches resulting from matching ambiguities (which may be detected by peak ratio Γ0 defined above). [sent-127, score-0.86]

46 Γ6(p) = |Dl1(p) − D2l(p)| Although not beneficial as a confidence measure itself, inclusion of disparity ambiguity into a learning framework is an attempt to separate small from large errors in image locations where the peak ratio may fail as explained above. [sent-128, score-1.081]

47 As an additional confidence measure, we use Zero mean Sum of Absolute Differences (ZSAD) matching costs between (left and right) image intensities Il and Ir for the winning disparity d1: Γ7(p) = ZSAD ? [sent-129, score-1.031]

48 Another proposal for confidence is what we call semi global × energy: We compute the sum of data and smoothness term in a small neighborhood for each pixel, choosing a patch size of 25 25 and aggregate along emerging rays in eight dsiizreec otfio 2n5s r f 2or5 t ahnedse a experiments. [sent-133, score-0.497]

49 gT ehem feeragtiunrge risa ydsef i nne edig hint analogy to the SGM objective energy, but with the winning disparity d1 = Dp fixed: Γ8(p) = ? [sent-134, score-0.454]

50 b1 and b2 are distinct penalties for different magnitudes of disparity map gradient, and t is a decision function. [sent-139, score-0.569]

51 333000777 Feature Vector Setup We define one feature vector f7 ∈ R7, containing only information derived from input images and computed disparity maps. [sent-140, score-0.418]

52 Features for lower scales are separately extracted from stereo computed on down-scaled images and not by downscaling of feature maps. [sent-143, score-0.447]

53 Vector f7 can be computed for arbitrary stereo results. [sent-145, score-0.447]

54 This feature vector is therefore defined only for stereo schemes with pixel-wise cost computations for each matching candidate. [sent-147, score-0.565]

55 Ensemble sures Learning for Confidence Mea- In the following, we explain the machine learning approach chosen for combining confidence measures. [sent-149, score-0.365]

56 We choose a classification approach instead of regression, as confidence measures do not contain matching error magnitude information as explained previously. [sent-152, score-0.637]

57 Each decision tree in the random forest partitions feature space recursively by greedily choosing a feature and a binary test thereupon, which minimizes an entropy based objective function. [sent-155, score-0.237]

58 Experiments Stereo estimates are computed using semi global matching stereo [11] (penalties b1 = 20, b2 = 100) with a binary census data term on 7 7 matching windows. [sent-164, score-0.813]

59 The choice cofe nthsuiss algorithm oisn d 7ue × ×to 7 b meastt cohvienrgal wl performance on unconstrained image data in terms of stereo accuracy [12, 21] as well as computational costs low enough for on-line results in, e. [sent-165, score-0.583]

60 We restrict our experiments to this powerful stereo algorithm, as we are not interested in stereo errors introduced through weak models. [sent-168, score-0.944]

61 In an effort to reduce adaptation to a specific matching problem domain, these frames are selected such that a variety of different challenges are posed to the stereo algorithm, including textureless areas, very large baseline, repetitive structures, transparencies and specular reflections. [sent-171, score-0.664]

62 Samples of the above described feature vector are collected only in locations where data term values for stereo matching are available (that is, these are not set to be invalid) on all scales and for all disparity candidates. [sent-173, score-0.954]

63 The intention is to avoid biases in learning and classification due to nonuniform scaling of some of the used cost function based features in the presence of undefined matching cost values. [sent-175, score-0.238]

64 Area under curve measures of our result (red), in comparison to four confidence measures that usually perform best. [sent-177, score-0.67]

65 As confidence measures generally contain no information about error magnitudes, solving a regression problem for feature combination is not likely to yield the intended results. [sent-180, score-0.548]

66 The class boundary is defined by a threshold of 3 px between ground truth disparities and stereo estimates, in line with the default of the KITTI online evaluation. [sent-182, score-0.534]

67 Due to very high quality of stereo results on KITTI in general, these two classes are highly unbalanced, which may deterioate class model quality and result in unnecesary computational costs due to high data volumes. [sent-184, score-0.538]

68 Generalisation error is monitored within the random forest framework by computing out of bag errors for increasingly large stratified random subsets of the training set. [sent-187, score-0.244]

69 Combined confidence measures for f7 and f23 alike are defined as the posterior probability of the bad disparity class. [sent-191, score-1.027]

70 Confidence measures, including decision forest results, are compared using the sparsification strategy: Pixels in disparity maps are successively removed, in the order of descending confidence measure values, until the disparity map is empty. [sent-192, score-1.498]

71 If the area under the resulting curve (AUC) is smaller than for concurrent confidence measures, it indicates that this measure is more accurate. [sent-194, score-0.437]

72 AUC values are normalized such that confidence measures discarding pixels randomly yield a value of 0. [sent-195, score-0.503]

73 Results Area under the curve (AUC) values for the proposed RDF23 confidence measure indicate superior accuracy compared to best performing of all single confidence measures on 193 out of 194 frames on the KITTI dataset, see Fig. [sent-198, score-1.005]

74 In the presence of frequent gross stereo errors which are generally detected well by all features including the semi global energy feature proposed, the RDF23 results still show a slight improvement, see Fig. [sent-203, score-0.668]

75 Even if a single contributing confidence measure fails (see Fig. [sent-205, score-0.512]

76 Outstanding accuracy gains from RDF23 results are not achieved if the confidence feature set is reduced to such 333000999 Figure 3. [sent-207, score-0.365]

77 Area under curve measures of our result when the feature set is reduced to information from disparity maps and image intensities. [sent-208, score-0.585]

78 Again, we compare to best performing single confidence measures. [sent-209, score-0.395]

79 variables that can be obtained solely from disparity maps and image intensities, assuming the stereo algorithm be a black box (see Fig. [sent-213, score-0.865]

80 In RDF23 estimation, disparity variance, perturbation, peak ratio and left-right difference have the largest contribution according to Gini importance in decision forest estimation (see Tab. [sent-216, score-0.739]

81 In the reduced feature set f7, Gini importance is highest for the disparity variance variable as well (see Tab. [sent-218, score-0.565]

82 Note, however, that stereo estimates are almost perfect for this frame. [sent-234, score-0.472]

83 despite the most important variable according to the Gini measure in both feature spaces being disparity variance. [sent-236, score-0.496]

84 The perturbation measure attracting higher variable importance on a smaller scale suggests that confidence may be more appropriate to be looked upon at superpixel level. [sent-237, score-0.579]

85 KITTI Frame 123, resulting in a significant amount of SGM stereo errors (approx. [sent-241, score-0.497]

86 30 percent), results in all confidence measures responding well. [sent-242, score-0.503]

87 Though one of the contributing measures, SGM energy, fails on Frame 151, our method results in superior accuracy compared to all single measures over the entire sparsification range. [sent-245, score-0.354]

88 For the only instance on KITTI Frame 30, error rates of the stereo algorithm are very low. [sent-248, score-0.492]

89 Undefined stereo values due to occluded regions cannot be handled separately in this study, as corresponding ground truth data is not yet made public in KITTI. [sent-251, score-0.472]

90 Yet, separate evaluations, as done in stereo benchmarking, would be of interest. [sent-253, score-0.447]

91 Conclusion We have demonstrated that learning a classifier on multivariate confidence measures is an appropriate approach to increase accuracy in stereo error detection if a suitable set of confidence features is selected. [sent-287, score-1.36]

92 In particular, variance based features on image intensities and matching results as previously applied to the optical flow problem are insufficient for consistently outperforming contributing confidence measures in stereo analysis. [sent-288, score-1.317]

93 Visualization of true positives (green), false positives (red), true negatives (blue) and false negatives (yellow) according to the denominations given in the plot of Fig. [sent-293, score-0.308]

94 flaws in the ground truth data [10] used here, advantages of the proposed method are larger where stereo is more challenging and hence produces more error prone results. [sent-296, score-0.517]

95 Yet, to shed light on this, new challenges for stereo need to be defined (and come with ground truth), beyond what is present in KITTI data. [sent-297, score-0.513]

96 This would help to shift attention to specific problems which need to be addressed before stereo vision systems can confidently be used in applicantions relevant to safety, such as driver assistance systems. [sent-299, score-0.447]

97 Quantitative evaluation of matching methods and validity measures for stereo vision. [sent-329, score-0.674]

98 A quantitative evaluation of confidence measures for stereo vision. [sent-381, score-0.95]

99 Binary confidence evaluation for a stereo vision based depth field processor SoC. [sent-419, score-0.84]

100 A simple stereo algorithm to recover precise object boundaries and smooth surfaces. [sent-425, score-0.447]


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