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unknown coecients of the fundamental solution for the equations (
α
), (
β
), and (
γ
)whichgovern
conformeomorphism by an equidistant map of the oblique meta-equator. In such a way, a boundary
value problem for the d'Alembert-Euler equations (Cauchy-Riemann equations) is defined and
solved. Finally, we show that special cases of the universal oblique Mercator projection for
2
A
1
,A
2
are normal Mercator and transverse Mercator. In addition, we shortly outline the local reduction
of the universal oblique Mercator projection of
E
A
1
,A
2
r
giveninBox
16.1
and as an
E
towards
S
example plotted in Fig.
16.1
(Fig.
16.2
).
S
r
, inclination
i
of a satellite orbit
Fig. 16.2.
Universal Oblique Mercator Projection of the sphere
Box 16.1 (The universal oblique Mercator projection of the sphere
r
.
α,β
: meta-longitude,
meta-latitude.
L, B
: longitude, latitude.
Ω,i
: longitude, inclination of the oblique meta-
equator).
S
x
=
rα
=
(16.1)
=
r
arctan[cos
i
tan(
L
−
Ω
)+sin
i
tan
B/
cos(
L
−
Ω
)]
,
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