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will be shown in the following. It will be also shown that the feature choice s I = 1
I 1
allow obtaining interaction matrices almost constant with respect to the depth dis-
tribution.
13.4.2.1
Variation with respect to Rotational Motion
Let us consider two frames
F 2 related to the unit sphere with different
orientations ( 1 R 2 is the rotation matrix between the two frames) but with the same
center. In this case, the value of I t isthesameforthetwoframes,sinceitisinvariant
to rotational motions. Let
F 1 and
X = 2 R 1 X
X
and
be the coordinates of a projected
point in the frame
F 1 and
F 2 respectively. Let us consider a function invariant to
rotations f (
X 1 ,...,X N ) that can be computed from the coordinates of N points
onto the unit sphere (such as the invariants computed from the projection onto the
unit sphere). The invariance condition between the frames
F 1 and
F 2 can thus be
written as
X 1 , ...,X N )= f ( 2 R 1 X 1 , ...,
2 R 1 X N )= f (
f (
X 1 , ...,X N )
.
(13.15)
The interaction matrix that links the variation of the function f with respect to trans-
lational velocities can be obtained as
L f v =
f (
X s 1 + T
,...,X N + T )
,
(13.16)
T
where T is a small translational motion vector. Let us now apply this formula for the
camera position defined by the frame
F 2 :
X 1 + T
,...,X N + T )
f ( 2 R 1 X 1 + T
2 R 1 X N + T ))
L f v =
T =
f
f (
=
,...,
.
(13.17)
T
T
From (13.17), it can be obtained that
f 2 R 1 (
X N + 1 R 2 T )
X 1 + 1 R 2 T )
2 R 1 (
L f v =
,...,
.
(13.18)
T
Combining this equation with the invariance to rotations condition (13.15), we get
X 1 + 1 R 2 T
,...,X N + 1 R 2 T )
L f v =
f (
.
(13.19)
T
From this, we easily obtain
X 1 + T ,...,X N + T )
T
L f v =
f (
(13.20)
T
T
where T = 1 R 2 T . Finally, combining (13.20) with (13.16), we obtain
L f v = L f v
1 R 2 .
(13.21)
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