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The constant Euclidean coordinates m j R
3
of the feature points expressed in
F c are defined as
m j = x 1 j ,
the camera frame
x 3 j T
x 2 j ,
.
These feature points, projected on the image plane
π i , are given by the constant
normalized coordinates m j R
3 as
x 1 j
x 3 j ,
1 T
x 2 j
x 3 j ,
m j =
.
(12.1)
3
The Euclidean coordinates m j ( t ) R
of the feature points expressed in the cam-
3
era frame
F c and the respective normalized Euclidean coordinates m j ( t ) R
are
defined as
m j ( t )= x 1 j ( t )
x 3 j ( t ) T
,
x 2 j ( t )
,
,
(12.2)
m j ( t )= x 1 j ( t )
1 T
x 2 j ( t )
x 3 j ( t ) ,
x 3 j ( t ) ,
.
(12.3)
3 . To facilitate the subsequent develop-
Consider a closed and bounded set
Y ⊂ R
ment, auxiliary state vectors y j =[ y 1 j ,
y 2 j ,
y 3 j ] T
∈ Y
and y j ( t )=[ y 1 j ( t ), y 2 j ( t ),
y 3 j ( t )] T
∈Y
are constructed from (12.1) and (12.3) as
y j = x 1 j
T
y j = x 1 j
T
x 2 j
x 3 j ,
1
x 3 j
x 2 j
x 3 j ,
1
x 3 j
x 3 j ,
x 3 j ,
.
(12.4)
The corresponding feature points m j and m j ( t ) viewed by the camera from two
different locations (and two different instances in time) are related by a depth ratio
α j ( t ) R
3
×
3 as
and a homography matrix H ( t ) R
R +
n T
x 3 j
x 3 j
x f
d
m j .
m j =
(12.5)
α j ( t )
H
Using projective geometry, the normalized Euclidean coordinates m j and m j ( t ) can
be related to the pixel coordinates in the image space as
p j = Am j
p j = Am j ,
(12.6)
where p j ( t )= u j v j 1 T
is a vector of the image-space feature point coordinates
3 is
a constant, known, invertible intrinsic camera calibration matrix [29]. Since A is
3 ,and A
3
×
R
I ⊂ R
R
u j ( t ), v j ( t )
defined on the closed and bounded set
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