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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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