announcements final exam friday, may 16 th 8am review session here, thursday 11am

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Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am.

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Page 1: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Announcements

Final Exam Friday, May 16th 8am

Review Session here, Thursday 11am.

Page 2: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Lighting affects appearance

Page 3: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am
Page 4: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am
Page 5: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Photometric Stereo: using this variability to reconstruct

Shape (normals only)Albedos

Page 6: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Recognition: Accounting for this variability in matching

Page 7: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Basics: How do we represent light? (1)

Ideal distant point source:

- No cast shadows

- Light distant

- Three parameters

- Example: lab with controlled

light

Page 8: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Basics: How do we represent light? (2)

Environment map: l( - Light from all directions

- Diffuse or point sources

- Still distant

- Still no cast shadows.

- Example: outdoors (sky and sun)

Sky

Page 9: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

`

Page 10: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Basics

How do objects reflect light?

Lambertian reflectance nl

lmax (cos, 0)

Page 11: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Reflectance map

Reflected light is function of surface normal: i = f(Suitable for environment map.

Can be measured with calibration object.

Page 12: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Photometric stereo

Given reflectance map:

i = f(each image constrains normal to one degree of freedom.

Given multiple images, solve at each point.

Page 13: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Lambertian + Point Source

Surface normal

Light

normal surface isˆ

is

radiance is

)ˆ(,0max(

light ofintensity is

light ofdirection is

n

albedo

i

nli

l

llll

Page 14: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Lambertian, point sources, no shadows. (Shashua, Moses)

Whiteboard

Solution linear

Linear ambiguity in recovering scaled normals

Lighting, reflectance map not known.

Recognition by linear combinations.

Page 15: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Linear basis for lighting

Z YX

Page 16: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Integrability

Means we can write height: z=f(x,y).

Whiteboard

Reduces ambiguity to bas-relief ambiguity.

Also useful in shape-from-shading and other photometric stereo.

Page 17: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Bas-relief Ambiguity

Page 18: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Shadows

Attached Shadow

Cast Shadow

Page 19: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

90.797.296.399.5#9

88.596.395.399.1#7

84.794.193.597.9#5

76.388.290.294.4#3

42.867.953.748.2#1

ParrotPhoneFaceBall

(Epstein, Hallinan and Yuille; see also Hallinan; Belhumeur and Kriegman)

5 2DDimension:

With Shadows: Empirical Study

Page 20: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Attached Shadows

Lambertian

Environment mapn

l

lmax (cos, 0)

Page 21: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Images

...

LightingReflectance

Page 22: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

0 1 2 30

0.5

1

0 1 2 30

0.5

1

1.5

2

r

Lighting to Reflectance: Intuition

Page 23: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am
Page 24: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

(See D’Zmura, ‘91; Ramamoorthi and Hanrahan ‘00)

Page 25: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Forming Harmonic Imagesnm nmb (p)=λr (X,Y,Z)

Z YX

2 2 22λ(Z -X -Y ) XZ YZ2 2λ(X -Y ) XY

Page 26: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Models

Query

Find Pose

Compare

Vector: IMatrix: B

Harmonic Images

Page 27: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Experiments 3-D Models of 42 faces

acquired with scanner.

30 query images for each of 10 faces (300 images).

Pose automatically computed using manually selected features (Blicher and Roy).

Best lighting found for each model; best fitting model wins.

Page 28: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am
Page 29: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Results

9D Linear Method: 90% correct.

9D Non-negative light: 88% correct.

Ongoing work: Most errors seem due to pose problems. With better poses, results seem near 97%.

Page 30: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am
Page 31: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am
Page 32: Announcements Final Exam Friday, May 16 th 8am Review Session here, Thursday 11am

Summary

Linear solutions are good.For pose variation with points, each image is linear combination of 2 others.For Lambertian lighting no shadows, each image is linear combination of 3.With attached shadows, linear combination of 9.Only diffuse lighting affects images, unless there are shadows or specularities.