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This makes sense; we've removed seven degrees of freedom (a similarity transfor-
mation) to fix the first camera, leaving eight degrees of freedom: the unknown five
entries of K 1 and the 3
1 vector c , which is related to the 3D projective distortion
of the environment. 18 Since K 1 is nonsingular, we can define a vector v
×
K
1
=−
c ,
so that
K 1
0
H
=
(6.46)
v K 1
1
Now, if we denote
P i =[
A i |
a i ]
(6.47)
K i K i
) 1 from Equation ( 6.23 ), it's straightforward
and recall the definition of
ω
= (
i
to show (see Problem 6.18 ) that
ω 1
i
a i v 1
a i v )
= (
A i
(
A i
1
P i
P i
ω 1
1
ω 1
1
v
=
(6.48)
v ω 1
1
v ω 1
1
v
P i QP i
Here, we have introduced a 4
4 symmetric matrix Q that depends only on the
elements of the transformation H . 19 T he equations in ( 6.48 ) are very important, since
they relate the projective camera matrices (which we know) to the elements of the
projective transformation H and the camera calibration matrices via
×
ω
i .
i , at this point we can impose constraints on
the form we wish it to take based on our knowledge about the camera calibration
matrices K i . These in turn impose constraints on Q through Equation ( 6.48 ).
For example, let's suppose the principal point is known to be
While we don't know the values of
ω
(
0, 0
)
and the aspect
ratio
α y x is known to be 1 — reasonable assumptions for a good camera. In this
case, only the focal length f i of each camera is unknown, and each
ω i has an extremely
simple form:
f 2 i 00
0 f 2 i 0
001
ω
=
(6.49)
i
So does the matrix Q :
q 1 00 q 2
0 q 1 0 q 3
001 q 4
q 2 q 3 q 4 q 5
Q
=
(6.50)
If we denote the rows of P i as P i , P i , P i and expand Equation ( 6.48 ) in this special
situation, we obtain four linear equations in the five unknowns of Q , corresponding
18 It is also related to what is called the plane at infinity for the projective reconstruction.
19 Q is also known as the absolute dual quadric [ 499 ].
 
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