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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