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P
:=
−
sin
B
0
cos
2
B
0
9
[1 + 2
E
2
(1
−
2cos
2
B
0
)] + O(
E
4
)
,
Q
:=
−
sin
B
0
36
[1 + 2
E
2
(1
5cos
2
B
0
)] + O(
E
4
)
,
−
A
I
AR
=
A
1
(1
−
E
2
)
S
E
2
A
1
A
2
5
l
F
(
b
N
− b
S
)+
B
9
l
E
(
b
N
− b
S
)+
(20.174)
b
S
)+O(8)
,
+
C
b
S
)+
D
b
S
)+
P
b
S
)+
Q
5
l
E
(
b
N
−
10
l
E
(
b
N
−
12
l
E
(
b
N
−
6
l
E
(
b
N
−
1
S
E
2
A
1
,A
2
=
2
E
2
sin
2
B
0
++sin
B
0
(1
2
E
2
sin
2
B
0
−
=
1
−
−
4
E
2
cos
2
B
0
)(
b
N
+
b
S
)
/
2cos
B
0
+O(
b
2
)
,
2
A
1
(1
−
E
2
)cos
B
0
l
E
(
b
N
−
b
S
)
(20.175)
A
b
N
−
b
S
b
N
−
b
S
1
2cos
B
0
5
l
E
+
B
b
S
l
E
+
C
I
AR
=
b
S
+
9
b
N
−
5
b
N
−
12
P
b
N
−
b
S
b
N
−
b
S
+
D
10
(
b
N
+
b
S
)
l
E
+
P
b
S
l
E
+
Q
×
(20.176)
b
N
−
6
b
N
−
b
S
2
E
2
sin
2
B
0
+sin
B
0
(1
2
E
2
sin
2
B
0
−
1
−
−
4
E
2
cos
2
B
0
)(
b
N
+
b
S
)
×
+O
R
(6)
,
2cos
B
0
b
S
)=
cos
4
B
0
360
(1 + 2
E
2
cos
2
B
0
+O(
E
4
))
l
E
+
I
AR
(
b
N
=
−
+
cos
2
B
0
324
(1 + O(
E
4
))
b
N
l
E
+
(1
−
2
E
2
cos
2
B
0
+O(
E
4
))
b
N
+O
R
(6)
.
(20.177)
360
End of Proof.
As an example, we compare in Table
20.5
the total deformation energy for conformal Gauss-
Krueger coordinates, parallel Soldner coordinates, and normal Riemann coordinates. Obviously,
in the range of application, normal Riemann coordinates generate the
smallest global distortion
,
followed by parallel Soldner coordinates (factor half compared to conformal Gauss-Krueger coor-
dinates), and conformal Gauss-Krueger coordinates.
Here, we take reference to G. B. Airy's definition of “balance of erros”. Conformal geodesics were
treated by
Beltrami
(
1869
),
Fialkow
(
1939
),
Legendre
(
1806
),
Schouten
(
1954
),
Vogel
(
1970
,
1973
),
Weingarten
(
1861
), and
Yano
(
1970
,
1940a
,
b
).
Boltz
(
1943
) presented formulae and tables for the
normal computation of Gauss-Krueger coordinates which we use here. For the optimal Universal
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