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H v [2]
Fig. 1.6 Multiple-view
geometry for the cameras
c 1 and c 2
1
v [1]
1
v [1 1
H v [1]
H v [2]
2
v [1]
1
2
v [2]
1
v [2 2
v [1]
2
H v [2]
2
v [1]
2
v [2 1
n 1
n 2
c 2
H R
c 1
From an inspection of Figure 1.6, it is easy to verify that the following equalities
hold true:
H R = H v [1]
= H v [2]
2
v [1]
1
2
v [2]
1
(1.16)
i.e. , the rigid motion between
c 1
and
c 2
is equal to the rigid motion between
v [1]
1
v [1]
2
v [2]
1
v [2]
2
and
, and between
and
. Using (1.16) and (1.14) into (1.15),
we obtain
H v [2]
H R = H v [2]
H v [2]
H v [2]
= H v [2]
H v [1]
H v [2]
H R H v [2]
= H v [2]
H 1
R
= H 1
R
v [1 2 ,
1
v [1]
1
1
v [2]
2
1
v [1]
1
2
v [2]
1
1
v [2]
2
2
v [1]
1
2
v [1]
2
2
v [1]
2
2
and (1.13) is thus proved.
Remark 1.2. Note that Equation 1.13 allows one to estimate the rigid motion H R
also when the epipolar geometry between
is not well-defined ( small
baseline case). In fact the epipolar geometry between the virtual cameras is always
well-defined by construction.
c 1
and
c 2
1.4
Mirror Calibration and Image-based Camera Localization
In this section we address the mirror calibration and image-based camera localiza-
tion problems using the PCS properties presented in Sections 1.2 and 1.3. Proposi-
tion 1.5 in the next section will be instrumental for Proposition 1.8 in Section 1.4.2.
1.4.1
Mirror Calibration
Consider the setup in Figure 1.4 and assume that at least n
2 points can be directly
observed by
c
at u i , i
∈{
1
,...,
n
}
. If the same set of points is also reflected by
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