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n 2 sin 2 arctan 1
c ( q 1 ) 2 +( q 2 ) 2 1 /n
1
d s 2 =
[(d q 1 ) 2 +(d q 2 ) 2 ] .
(E.59)
2
Box E.2 (The Lagrangean version versus the Hamiltonian version of a geodesic in
S
R in terms
of conformal coordinates (isometric coordinates) and Maupertuis gauge).
(i) Universal Polar Stereographic Projection (UPS):
L 2 ( q ( t ) , q ( t )) = 1
8 R 4
(4 R 2 +( q 1 ) 2 +( q 2 ) 2 ) 2 ,
2 δ μν q μ q ν +
(E.60)
8 R 4
(4 R 2 +( q 1 ) 2 +( q 2 ) 2 ) 2 .
(ii) Universal Mercator Projection (UM):
L 2 ( q ( t ) , q ( t )) = 1
H 2 ( q ( t ) ,p ( t )) = 1
2 ( p 1 + p 2 )
2cosh 2 ( q 2 /R ) ,H 2 ( q ( t ) ,p ( t )) = 1
1
2 δ μν q μ q ν +
2 ( p 1 + p 2 )
1
2cosh 2 ( q 2 /R ) .
(E.61)
(iii) Universal Transverse Mercator Projection (UTM):
L 2 ( q ( t ) , q ( t )) = 1
2 δ μν q μ q ν + 1
2 cos 2 arcsin[tanh( q 2 /R )] ,
(E.62)
H 2 ( q ( t ) ,p ( t )) = 1
1
2 cos 2 arcsin[tanh( q 2 /R )] .
(iv) Universal Conic Projection (UC):
L 2 ( q ( t ) , q ( t )) 1
2 ( p 1 + p 2 )
2 n sin 2 arctan 1
c ( q 1 ) 2 +( q 2 ) 2 1 /n
1
2 δ μν q μ q ν +
,
(E.63)
2 n sin 2 arctan 1
c ( q 1 ) 2 +( q 2 ) 2 1 /n
H 2 ( q ( t ) ,p ( t )) = 1
1
2 ( p 1 + p 2 )
.
2
Box E.3 (The differential equations of a geodesic in
R in terms of conformal coordinates
(isometric coordinates) and Maupertuis gauge: Lagrange portrait, two differential equations
of second order, Hamilton portrait, four differential equations of first order).
(i) Universal Polar Stereographic Projection (UPS):
S
32 R 4
q μ +
(4 R 2 +( q 1 ) 2 +( q 2 ) 2 ) 3 q μ =0
μ =1 , 2 ,
q μ = δ μν p ν
μ, ν =1 , 2
(E.64)
(summation convention),
 
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