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positioning error introduced by image measurement errors. For this reason, from
now on we will consider the computation of the errors
s
r
(
δ
) and
s
t
(
δ
) where
δ
,
defined as
ζ
,
δ
=
ε
+ 2
(9.11)
represents the total image error.
Before proceeding, let us parameterize the rotation matrix through the Cayley
parameter. Let us define the function
3
3
×
3
Γ
:
R
→
R
(
a
)=
I
3
−
1
I
3
+[
a
]
Γ
−
[
a
]
×
(9.12)
×
3
is called Cayley parameter. It turns out that this
parametrization satisfies the following properties:
1.
a
3
)
T
where
a
=(
a
1
,
a
2
,
∈
R
3
;
∈
∈
R
Γ
(
a
)
SO
(3) for all
a
3
∈
θ
<
π
∈
R
2. for any
R
SO
(3) such that
θ
in (9.8) satisfies
, there exists
a
such
(
a
).
Moreover, (9.12) can be rewritten as
that
R
=
Γ
(
a
)=
Ω
(
a
)
Γ
(9.13)
2
1 +
a
3
×
3
is the matrix quadratic polynomial given by
3
where
Ω
(
a
) :
R
→
R
⎛
⎞
a
1
−
a
2
−
a
3
+ 12(
a
1
a
2
−
a
3
)
2 (
a
1
a
3
+
a
2
)
⎝
⎠
.
a
1
+
a
2
−
a
3
+ 12(
a
2
a
3
−
−
Ω
(
a
)=
2 (
a
1
a
2
+
a
3
)
a
1
)
(9.14)
a
1
−
a
2
+
a
3
+ 1
2 (
a
1
a
3
−
a
2
)
2 (
a
2
a
3
+
a
1
)
−
9.3.1
Upper Bounds
Let us consider first the computation of upper bounds of
s
r
(
) in (9.7)-
(9.9). We will show that this step can be solved by exploiting convex optimization.
Indeed, consider the constraint
δ
) and
s
t
(
δ
p
∗
∞
<
δ
p
−
in the computation of
s
r
(
δ
) and
s
t
(
δ
).
From (9.1), (9.3) and (9.5) it follows that for the
i
-th point we can write
(
a
)
T
q
i
(
a
)
T
t
Ω
−
Ω
q
i
e
3
q
i
p
∗
i
=
A
p
i
−
(
a
)
T
t
)
−
A
(9.15)
e
3
(
Ω
(
a
)
T
q
i
−
Ω
where it has been taken into account that
q
i
is expressed with respect to the desired
camera frame
F
∗
, which coincides with the absolute frame
F
abs
. Hence, we have that
p
∗
i
∞
≤
δ
p
i
−
if and only if
⎧
⎨
|
f
i
,
3
g
i
,
1
(
a
,
t
)
−
f
i
,
1
g
i
,
3
(
a
,
t
)
|≤
δ
f
i
,
3
g
i
,
3
(
a
,
t
)
|
f
i
,
3
g
i
,
2
(
a
,
t
)
−
f
i
,
2
g
i
,
3
(
a
,
t
)
|≤
δ
f
i
,
3
g
i
,
3
(
a
,
t
)
(9.16)
⎩
g
i
,
3
(
a
,
t
)
>
0
where
f
i
,
j
∈
R
is a constant and
g
i
,
j
(
a
,
t
) is a polynomial given by
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