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Stereo EECS 442 Prof. David Fouhey Winter 2019, University of - PowerPoint PPT Presentation

Stereo EECS 442 Prof. David Fouhey Winter 2019, University of Michigan http://web.eecs.umich.edu/~fouhey/teaching/EECS442_W19/ Congrats to P2 Kaggle Winners (Gold) William Dong (0.673) (Silver) Chockalingam Ravi Sundaram (0.669)


  1. Stereo EECS 442 – Prof. David Fouhey Winter 2019, University of Michigan http://web.eecs.umich.edu/~fouhey/teaching/EECS442_W19/

  2. Congrats to P2 Kaggle Winners • (Gold) William Dong (0.673) • (Silver) Chockalingam Ravi Sundaram (0.669) • (Bronze) VentusYue (0.662) • Top-10: Hongzhi Yang, junzhexu, Shadow Demon, Izzy P, Mega Flygon, Naive, and goblue

  3. Two-View Stereo Slide credit: S. Seitz

  4. Stereo Slide credit: S. Lazebnik

  5. https://petapixel.com/2018/03/07/two-photographers-unknowingly-shot-millisecond-time/

  6. https://petapixel.com/2018/03/07/two-photographers-unknowingly-shot-millisecond-time/

  7. https://petapixel.com/2018/03/07/two-photographers-unknowingly-shot-millisecond-time/

  8. Stereograms Humans can fuse pairs of images to get a sensation of depth Stereograms: Invented by Sir Charles Wheatstone, 1838 Slide credit: S. Lazebnik

  9. Stereograms Slide credit: S. Lazebnik

  10. Stereograms What about this? Slide Credit: S. Lazebnik, but idea of random dot sterogram is due to B. Julesz

  11. Stereograms Bela Julesz: Random Dot Stereogram Shows that stereo can operate without recognition Slide Credit: S. Lazebnik, but idea of random dot sterogram is due to B. Julesz

  12. Stereograms Humans can fuse pairs of images to get a sensation of depth Autostereograms: www.magiceye.com Slide credit: S. Lazebnik

  13. Stereograms Humans can fuse pairs of images to get a sensation of depth Autostereograms: www.magiceye.com Slide credit: S. Lazebnik

  14. Problem formulation Given a calibrated binocular stereo pair, fuse it to produce a depth image image 1 image 2 Dense depth map Slide credit: S. Lazebnik

  15. Basic stereo matching algorithm • For each pixel in the first image • Find corresponding epipolar line in the right image • Examine all pixels on the epipolar line and pick the best match • Triangulate the matches to get depth information • Simplest case: epipolar lines = corresponding scanlines • When does this happen? Slide credit: S. Lazebnik

  16. Simplest Case: Parallel images • Image planes of cameras are parallel to each other and to the baseline • Camera centers are at same height • Focal lengths the same Slide credit: S. Lazebnik

  17. Simplest Case: Parallel images • Image planes of cameras are parallel to each other and to the baseline • Camera centers are at same height • Focal lengths the same • Then epipolar lines fall along the horizontal scan lines of the images Slide credit: S. Lazebnik

  18. Essential matrix for parallel images 𝒒𝑭𝒒 ′ = 0 𝑭 = 𝒖 𝒚 𝑺 What’s R? What’s t? p 𝑺 = 𝑱 𝑢 = [𝑈, 0,0] 0 0 0 p' y 𝑭 = 𝒖 𝒚 𝑺 = z 0 0 −𝑈 T 0 𝑈 0 x 0 −𝑈𝑤 + 𝑈 ′ 𝑤 = 0 0 0 0 𝑣′ 𝑣 𝑤 1 = 0 𝑣 𝑤 1 = 0 −𝑈 0 0 −𝑈 𝑤′ 𝑈 ′ 𝑤 = 𝑈𝑤 𝑈 ′ 𝑤 0 𝑈 0 1 The y-coordinates of corresponding points are the same! Slide credit: S. Lazebnik

  19. Stereo image rectification Slide credit: S. Lazebnik

  20. Stereo image rectification Reproject image planes onto a common plane parallel to the line between optical centers C. Loop and Z. Zhang. Computing Rectifying Homographies for Stereo Vision. CVPR 1999 Slide credit: S. Lazebnik

  21. Rectification example Slide credit: S. Lazebnik

  22. Another rectification example Unrectified Rectified Slide credit: S. Lazebnik

  23. Basic stereo matching algorithm • If necessary, rectify the two stereo images to transform epipolar lines into scanlines • For each pixel in the first image • Find corresponding epipolar line in the right image • Examine all pixels on the epipolar line and pick the best match Slide credit: S. Lazebnik

  24. Correspondence Search Left Right scanline Matching cost disparity Slide window along the right scanline, compare contents of that window with reference window on left Matching cost: SSD or normalized correlation Slide credit: S. Lazebnik

  25. Correspondence Search Left Right scanline Matching cost Sum of squared differences 𝑗 2 ෍ 𝑚 𝑗 − 𝑠 𝑗 Disparity Slide credit: S. Lazebnik

  26. Correspondence Search Left Right scanline Matching cost Normalized correlation መ 𝑦 𝑗 = 𝑦 𝑗 − mean 𝑦 𝑚 ⋅ Ƹ 𝑠 ෝ std(𝑦) Disparity Slide credit: S. Lazebnik

  27. Basic stereo matching algorithm • If necessary, rectify the two stereo images to transform epipolar lines into scanlines • For each pixel x in the first image • Find corresponding epipolar scanline in the right image • Examine all pixels on the scanline and pick the best match x ’ • Triangulate the matches to get depth information Slide credit: S. Lazebnik

  28. Triangulation: Older History • From Wikipedia: Gemma Frisius's 1533 diagram introducing the idea of triangulation into the science of surveying. Having established a baseline, e.g. the cities of Brussels and Antwerp, the location of other cities, e.g. Middelburg, Ghent etc., can be found by taking a compass direction from each end of the baseline, and plotting where the two directions cross. This was only a theoretical presentation of the concept — due to topographical restrictions, it is impossible to see Middelburg from either Brussels or Antwerp. Nevertheless, the figure soon became well known all across Europe. Slide credit: S. Lazebnik

  29. Triangulation: Modern History

  30. Depth from disparity 𝑔 = 𝐶 1 𝑦 𝑨 By similar triangles z −𝑦′ 𝑔 = 𝐶 2 x x' 𝑨 f f B 1 B 2 Similarly by o o' similar triangles Diagram adapted from S. Lazebnik

  31. Depth from disparity 𝑔 = 𝐶 1 𝑦 −𝑦′ 𝑔 = 𝐶 2 𝑨 𝑨 Add them 𝑦 − 𝑦′ = 𝐶 1 + 𝐶 2 z x x' 𝑔 𝑨 f f 𝑦 − 𝑦′ = 𝑔𝐶 B 1 B 2 𝑨 Baseline B o o' B=B 1 +B 2 Disparity Diagram adapted from S. Lazebnik

  32. Depth from disparity 𝑔 = 𝐶 1 𝑦 𝑦′ 𝑔 = 𝐶 2 𝑨 𝑨 Subtract them 𝑦 − 𝑦′ = 𝐶 1 − 𝐶 2 z x x' 𝑔 𝑨 f f 𝑦 − 𝑦′ = 𝑔𝐶 B o o' 𝑨 B 1 B 2 Diagram adapted from S. Lazebnik

  33. Basic stereo matching algorithm • If necessary, rectify the two stereo images to transform epipolar lines into scanlines • For each pixel x in the first image • Find corresponding epipolar scanline in the right image • Examine all pixels on the scanline and pick the best match x ’ • Compute disparity x –x’ and set depth( x ) = B * f /( x –x’ ) Slide credit: S. Lazebnik

  34. Failures of Correspondence Search Textureless regions. Why? ? ? ? ? Image credit: S. Lazebnik

  35. Failures of Correspondence Search Repeated Patterns. Why? ? ? Image credit: S. Lazebnik

  36. Failures of Correspondence Search Specular Surfaces. Why? Image credit: S. Lazebnik

  37. Effect of window size W = 3 W = 20 • Smaller window + More detail - More noise • Larger window + Smoother disparity maps - Less detail Image credit: S. Lazebnik

  38. Results with window search Data Ground truth Window-based matching Image credit: S. Lazebnik

  39. Better methods exist... Graph cuts Ground truth Y. Boykov, O. Veksler, and R. Zabih, Fast Approximate Energy Minimization via Graph Cuts, PAMI 2001 For the latest and greatest: http://www.middlebury.edu/stereo/ Image credit: S. Lazebnik

  40. Improving Window-based Matching • Similarity is local (each window independent) • Need non-local correspondence constraints / cues.

  41. Uniqueness • Each point in one image should match at most one point in other image. • When might this not be true? o o'

  42. Ordering • Corresponding points should be in same order a b c abc abc o o'

  43. Ordering • Not always true! a b c d abdc adbc o o'

  44. Smoothness • We expect disparity values to change slowly (for the most part) • When is this not true?

  45. Scanline Stereo • Try to coherently match pixels on the entire scanline • Different scanlines are optimized (by dynamic programming) independently Left image Right image Slide credit: S. Lazebnik

  46. “Shortest paths” for scan -line stereo I  Left image Right image I S left Right occlusion C q occl occlusion Left t C C corr occl S right s p Can be implemented with dynamic programming Ohta & Kanade ’85, Cox et al. ‘96 Slide credit: Y. Boykov

  47. Coherent Stereo on 2D Grid • Scanline stereo generates streaking artifacts • Can’t use dynamic programming to find spatially coherent disparities on a 2D grid Slide credit: S. Lazebnik

  48. Stereo Matching as Optimization I 2 D I 1 W 1 ( i ) W 2 ( i+D ( i )) D ( i ) 2 𝐹 𝐸 = ෍ 𝑋 1 𝑗 − 𝑋 2 𝑗 + 𝐸 𝑗 + 𝜇 ෍ 𝜍 𝐸 𝑗 − 𝐸(𝑘) 𝑗 neighbors 𝑗,𝑘 Smoothness term Data term Solvable by graph cuts for certain smoothnesses ρ Y. Boykov, O. Veksler, and R. Zabih, Fast Approximate Energy Minimization via Graph Cuts, PAMI 2001 Slide credit: S. Lazebnik

  49. Is This Doable by Deep Network? I 2 D I 1 W 1 ( i ) W 2 ( i+D ( i )) D ( i ) 2 𝐹 𝐸 = ෍ 𝑋 1 𝑗 − 𝑋 2 𝑗 + 𝐸 𝑗 + 𝜇 ෍ 𝜍 𝐸 𝑗 − 𝐸(𝑘) 𝑗 neighbors 𝑗,𝑘 Smoothness term Data term Easy solution: replace the data term with a network

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