Geography Reference
In-Depth Information
Box 8.4 (Two ellipsoidal coordinate systems parameterizing the oblate ellipsoid-of-
revolution).
Oblate ellipsoid-of-revolution:
A
1
,A
2
,A
3
:=
X
+
.
X
2
+
Y
2
A
1
+
Z
2
3
E
∈
R
|
A
2
=1
,A
1
>A
2
∈
R
(8.28)
Ansatz 1 (surface normal coordinates):
Ansatz 2 (circle reduced coordinates):
X
=
A
1
cos
Φ
cos
Λ
√
1
−E
2
sin
2
Φ
,
X
=
A
1
cos
Φ
∗
cos
Λ,
Y
=
A
1
cos
Φ
sin
Λ
√
1
−E
2
sin
2
Φ
,
Y
=
A
1
cos
Φ
∗
sin
Λ,
(8.29)
Z
=
A
1
(1
−
E
2
)sin
Φ
√
1
−E
2
sin
2
Φ
,
Z
=
A
2
sin
Φ
∗
,
subject to
A
1
=
√
1
E
2
:=
A
1
−
A
2
A
2
and
−
E
2
.
(8.30)
A
1
Direct and inverse transformation of surface normal latitude
Φ
to circle reduced latitude
Φ
∗
:
1
1
−E
2
Z
√
X
2
+
Y
2
versus tan
Φ
∗
=
A
1
Z
√
X
2
+
Y
2
tan
Φ
=
A
2
1
√
1
−E
2
Z
=
√
X
2
+
Y
2
,
versus tan
Φ
∗
=
√
1
√
1
−E
2
tan
Φ
∗
1
tan
Φ
=
−
E
2
tan
Φ,
(8.31)
√
1
−E
2
√
1
−E
2
cos
2
Φ
∗
cos
Φ
∗
versus
cos
Φ
∗
=
√
1
−
E
2
sin
2
Φ
cos
Φ,
1
cos
Φ
=
√
1
√
1
−E
2
√
1
−E
2
sin
2
Φ
sin
Φ.
sin
Φ
=
E
2
cos
2
Φ
∗
sin
Φ
∗
versus
sin
Φ
∗
=
√
1
−
In most practical cases, where we are aiming at an azimuthal projection of an equidistant type
of the ellipsoid-of-revolution representing the Earth, the planets, or other celestial bodies, a series
expansion of the meridian arc length has been a sucient approximation. Accordingly, we are
going to outline the series expansion of the meridian arc length as a function of surface normal lati-
tude
Φ
or its complement, the polar distance
Δ
. In preparing such an series expansion, we have col-
lected auxiliary formulae in Corollaries
8.1
to
8.7
.First,weexpand(1+
x
)
y
according to B.Taylor,
just representing the meridian arc length by
x
:=
E
2
cos 2
Δ, y
=
−
−
3
/
2, and
|
x
|
>
1. Second,
E
2
cos
2
Δ
)
3
/
2
in terms of powers
1
,E
2
cos
2
Δ, E
4
cos
4
Δ, E
6
cos
6
Δ,...
we represent (1
−
{
}
.Third,
cos
2
Δ,
cos
4
Δ,
cos
6
Δ,...
we transform the powers
.
Fourth, an explicit version of the product sums is given in Corollaries
8.4
to
8.6
. Since the power
series are
uniformly convergent
, we can term-wise integrate in order to achieve the meridian arc
length in Corollary
8.7
.
{
}
in terms of
{
1
,
cos2
Δ,
cos 4
Δ,
cos 6
Δ,...
}
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