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A
2
cos
2
r
−
1
((
q
1
)
2
+(
q
2
)
2
)
d
s
2
=
c
2
n
2
1
e
2
sin
2
r
−
1
(
q
1
)
2
+(
q
2
)
2
×
(E.89)
−
r
−
1
(
q
1
)
2
+(
q
2
)
2
⎛
⎝
tan
2
⎛
⎞
π
4
−
⎝
⎠
×
2
1+
e
sin
r
−
1
(
q
1
)
2
+(
q
2
)
2
1
− e
sin
r
−
1
(
q
1
)
2
+(
q
2
)
2
⎛
⎞
⎞
−n
e
(
q
1
)
2
+(
q
2
)
2
.
⎝
⎠
⎠
(
λ
(
q
1
.q
2
) from series inversion of
q
1
(
Λ, Φ
)and
q
2
(
Λ, Φ
) leading to
Λ
(
q
1
,q
2
)and
Φ
(
q
1
,q
2
).
See
Snyder
(
1987a
, p. 109).
Box E.5 (The Lagrangean version versus the Hamiltonian version of a geodesic in
E
2
A,B
in
terms of conformal coordinates (isometric coordinates) and Maupertuis gauge).
(i)Universal Polar Stereographic Projection (UPS):
L
2
(
q
(
t
)
, q
(
t
)) =
1
2
(
q
1
)
2
+(
q
2
)
2
A
2
cos
2
f
−
1
(
q
1
)
2
+(
q
2
)
2
2
1
1
(
q
1
)
2
+(
q
2
)
2
,
e
2
sin
2
f
1
(
q
1
)
2
+(
q
2
)
2
+
(E.90)
−
H
2
(
q
(
t
)
,p
(
t
)) =
1
2
(
p
1
+
p
2
)
A
2
cos
2
f
−
1
(
q
1
)
2
+(
q
2
)
2
2
1
− e
2
sin
2
f
1
(
q
1
)
2
+(
q
2
)
2
1
(
q
1
)
2
+(
q
2
)
2
.
−
(E.91)
(ii)Universal Mercator Projection (UM):
L
2
(
q
(
t
)
, q
(
t
)) =
1
2
(
q
1
)
2
+(
q
2
)
2
+
1
e
2
sin
2
f
1
(
q
2
/A
)
2cos
2
f
−
1
(
q
2
/A
)
−
,
(E.92)
e
2
sin
2
f
−
1
(
q
2
/A
)
2cos
2
f
1
(
q
2
/A
)
H
2
(
q
(
t
)
,p
(
t
)) =
1
1
−
2
(
p
1
+
p
2
)
−
.
(E.93)
(iii)Universal Transverse Mercator Projection (UTM):
L
2
(
q
(
t
)
, q
(
t
)) =
1
2
[(
q
1
)
2
+(
q
2
)
2
]+
1
2
ρ
2
(1 +
d
02
(
q
2
)
2
+
d
12
q
1
(
q
2
)
2
+
d
22
(
q
1
)
2
(
q
2
)
2
+
(E.94)
+
d
32
(
q
1
)
3
(
q
2
)
2
+
d
04
(
q
2
)
4
+
d
14
q
1
(
q
2
)
4
+O
λ
2
((
q
1
)
6
,
(
q
2
)
6
))
,
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