1. Analysis of Lighting Effects Outline: The problem Lighting models Shape from shading Photometric stereo Harmonic analysis of lighting

5. Applications Modeling the effect of lighting can be used for Recognition – particularly face recognition Shape reconstruction Motion estimation Re-rendering …

6. Lighting is Complex Lighting can come from any direction and at any strength Infinite degree of freedom

7. Issues in Lighting Single light source (point, extended) vs. multiple light sources Far light vs. near light Matt surfaces vs. specular surfaces Cast shadows Inter-reflections

8. Lighting From a source – travels in straight lines Energy decreases with r 2 (r – distance from source) When light rays reach an object  Part of the energy is absorbed  Part is reflected (possibly different amounts in different directions)  Part may continue traveling into the object, if object is transparent / translucent

9. Specular Reflectance When a surface is smooth light reflects in the opposite direction of the surface normal

10. Specular Reflectance When a surface is slightly rough the reflected light will fall off around the specular direction

11. Lambertian Reflectance When the surface is very rough light may be reflected equally in all directions

12. Lambertian Reflectance When the surface is very rough light may be reflected equally in all directions

13. Lambertian Reflectance

14. Lambert Law or 

15. BRDF A general description of how opaque objects reflect light is given by the Bidirectional Reflectance Distribution Function (BRDF) BRDF specifies for a unit of incoming light in a direction (θ i,Φ i ) how much light will be reflected in a direction (θ e,Φ e ). BRDF is a function of 4 variables f(θ i,Φ i ;θ e,Φ e ). (0,0) denotes the direction of the surface normal. Most surfaces are isotropic, i.e., reflectance in any direction depends on the relative direction with respect to the incoming direction (leaving 3 parameters)

16. Why BRDF is Needed? Light from front Light from back

17. Most Existing Algorithms Assume a single, distant point source All normals visible to the source (θ<90°) Plus, maybe, ambient light (constant lighting from all directions)

18. Shape from Shading Input: a single image Output: 3D shape Problem is ill-posed, many different shapes can give rise to same image Common assumptions:  Lighting is known  Reflectance properties are completely known – For Lambertian surfaces albedo is known (usually uniform)

19. convex concave

20. convex concave

21. HVS Assumes Light from Above

23. Lambertian Shape from Shading (SFS) Image irradiance equation Image intensity depends on surface orientation It also depends on lighting and albedo, but those assumed to be known

24. Surface Normal A surface z(x,y) A point on the surface: (x,y,z(x,y)) T Tangent directions t x =(1,0,p) T, t y =(0,1,q) T with p=z x, q=z y

25. Lambertian SFS We obtain Proportionality – because albedo is known up to scale For each point one differential equation in two unknowns, p and q But both come from an integrable surface z(x,y) Thus, p y = q x (z xy =z yx ). Therefore, one differential equation in one unknowns

26. Lambertian SFS

27. SFS with Fast Marching Suppose lighting coincides with viewing direction l=(0,0,1) T, then Therefore For general l we can rotate the camera

28. Distance Transform is called Eikonal equation Consider d(x) s.t. |d x |=1 Assume x 0 =0 x0x0 d x

29. Distance Transform is called Eikonal equation Consider d(x) s.t. |d x |=1 Assume x 0 =0 and x 0 =1 x0x0 d x x1x1

30. SFS with Fast Marching - Some places are more difficult to walk than others Solution to Eikonal equations –using a variation of Dijkstra’s algorithm Initial condition: we need to know z at extrema Starting from lowest points, we propagate a wave front, where we gradually compute new values of z from old ones

31. Results

32. Photometric Stereo Fewer assumptions are needed if we have several images of the same object under different lightings In this case we can solve for both lighting, albedo, and shape This can be done by Factorization Recall that Ignore the case θ>90°

33. Photometric Stereo - Factorization Goal: given M, find L and S What should rank(M) be?

34. Photometric Stereo - Factorization Use SVD to find a rank 3 approximation Define So Factorization is not unique, since, A invertible To reduce ambiguity we impose integrability

35. Reducing Ambiguity Assume We want to enforce integrability Notice that Denote by the three rows of A, then From which we obtain

36. Reducing Ambiguity Linear transformations of a surface It can be shown that this is the only transformation that maintains integrability Such transformations are called “generalized bas relief transformations” (GBR) Thus, by imposing integrability the surface is reconstructed up to GBR

37. Relief Sculptures

38. Illumination Cone Due to additivity, the set of images of an object under different lighting forms a convex cone in R N This characterization is generic, holds also with specularities, shadows and inter-reflections Unfortunately, representing the cone is complicated (infinite degree of freedom) = 0.5*+0.2*+0.3*

39. Eigenfaces Photobook/Eigenfaces (MIT Media Lab)

40. Recognition with PCA Amano, Hiura, Yamaguti, and Inokuchi; Atick and Redlich; Bakry, Abo-Elsoud, and Kamel; Belhumeur, Hespanha, and Kriegman; Bhatnagar, Shaw, and Williams; Black and Jepson; Brennan and Principe; Campbell and Flynn; Casasent, Sipe and Talukder; Chan, Nasrabadi and Torrieri; Chung, Kee and Kim; Cootes, Taylor, Cooper and Graham; Covell; Cui and Weng; Daily and Cottrell; Demir, Akarun, and Alpaydin; Duta, Jain and Dubuisson-Jolly; Hallinan; Han and Tewfik; Jebara and Pentland; Kagesawa, Ueno, Kasushi, and Kashiwagi; King and Xu; Kalocsai, Zhao, and Elagin; Lee, Jung, Kwon and Hong; Liu and Wechsler; Menser and Muller; Moghaddam; Moon and Philips; Murase and Nayar; Nishino, Sato, and Ikeuchi; Novak, and Owirka; Nishino, Sato, and Ikeuchi; Ohta, Kohtaro and Ikeuchi; Ong and Gong; Penev and Atick; Penev and Sirivitch; Lorente and Torres; Pentland, Moghaddam, and Starner; Ramanathan, Sum, and Soon; Reiter and Matas; Romdhani, Gong and Psarrou; Shan, Gao, Chen, and Ma; Shen, Fu, Xu, Hsu, Chang, and Meng; Sirivitch and Kirby; Song, Chang, and Shaowei; Torres, Reutter, and Lorente; Turk and Pentland; Watta, Gandhi, and Lakshmanan; Weng and Chen; Yuela, Dai, and Feng; Yuille, Snow, Epstein, and Belhumeur; Zhao, Chellappa, and Krishnaswamy; Zhao and Yang…

41. BallFacePhoneParrot #148.253.767.942.8 #284.475.283.269.7 #394.490.288.276.3 #496.592.192.081.5 #597.993.594.184.7 #698.994.595.287.2 #799.195.396.388.5 #899.395.896.889.7 #999.596.397.290.7 #1099.696.697.591.7 Empirical Study (Yuille et al.)

42. lighting reflectance Intuition

43.    (Light → Reflectance) = Convolution

44.   

45. Spherical Harmonics  ZYX XZYZXY Positive values Negative values

46. Harmonic Transform of Kernel n

47. Cumulative Energy N (percents)

48. Second Order Approximation

49. Reflectance Near 9D Yields 9D linear subspace. 4D approximation (first order) can also be used = point source + ambient

50. Harmonic Representations  Positive values Negative values ρ Albedo n Surface normal

51. Photometric Stereo L M S Image n : Image 1 Light n : Light 1 * SVD recovers L and S up to an ambiguity  nznz nznz nyny  n z 2 -1)  n x 2 -n y 2 ) nxnynxny nxnznxnz nynznynz

52. Photometric Stereo

54. Summary Lighting effects are complex Algorithms for SFS and photometric stereo for Lambertian object illuminated by a single light source Harmonic analysis extends this to multiple light sources Handling specularities, shadows, and inter- reflections is difficult

55. Mutual Information Camera Rotation