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ECE 549CS 543: COMPUTER VISON LECTURE 14

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Properties of the Essential Matrix. E p' is the epipolar line associated with p' ... Ignore the non-linear constraints and use linear least-squares. a posteriori. ... – PowerPoint PPT presentation

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Title: ECE 549CS 543: COMPUTER VISON LECTURE 14


1
ECE 549/CS 543 COMPUTER VISON LECTURE
14 MULTI-VIEW GEOMETRY II
  • The Essential Matrix
  • The Fundamental Matrix
  • The 8-Point Algorithm
  • The Trifocal Tensor
  • Reading Chapter 10
  • A list of potential projects is at
  • http//www-cvr.ai.uiuc.edu/ponce/fall04/project
    s.pdf
  • Homework Weak Calibration due Th. Oct. 21.
  • http//www-cvr.ai.uiuc.edu/ponce/fall04/hw3/hw3
    .pdf


2
Epipolar Constraint Calibrated Case
Essential Matrix (Longuet-Higgins, 1981)
3
Properties of the Essential Matrix
  • E p is the epipolar line associated with p.
  • E p is the epipolar line associated with p.
  • E e0 and E e0.
  • E is singular.
  • E has two equal non-zero singular values
  • (Huang and Faugeras, 1989).

T
T
4
Epipolar Constraint Uncalibrated Case
Fundamental Matrix (Faugeras and Luong, 1992)
5
Properties of the Fundamental Matrix
  • F p is the epipolar line associated with p.
  • F p is the epipolar line associated with p.
  • F e0 and F e0.
  • F is singular.

T
T
6
The Eight-Point Algorithm (Longuet-Higgins, 1981)
7
Non-Linear Least-Squares Approach (Luong et al.,
1993)
Minimize
with respect to the coefficients of F , using an
appropriate rank-2 parameterization.
8
The Normalized Eight-Point Algorithm (Hartley,
1995)
  • Center the image data at the origin, and scale
    it so the
  • mean squared distance between the origin and the
    data
  • points is 2 pixels q T p , q T p.
  • Use the eight-point algorithm to compute F from
    the
  • points q and q .
  • Enforce the rank-2 constraint.
  • Output T F T.

i
i
i
i
i
i
T
9
Data courtesy of R. Mohr and B. Boufama.
10
Mean errors 10.0pixel 9.1pixel
Without normalization
Mean errors 1.0pixel 0.9pixel
With normalization
11
Trinocular Epipolar Constraints
These constraints are not independent!
12
Trinocular Epipolar Constraints Transfer
Given p and p , p can be computed as the
solution of linear equations.
1
2
3
13
Trifocal Constraints
14
Trifocal Constraints
Calibrated Case
All 3x3 minors must be zero!
Trifocal Tensor
15
Trifocal Constraints
Uncalibrated Case
Trifocal Tensor
16
Properties of the Trifocal Tensor
i
1
Estimating the Trifocal Tensor
  • Ignore the non-linear constraints and use linear
    least-squares
  • a posteriori.
  • Impose the constraints a posteriori.

17
The backprojections of the two lines do not
define a line!
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