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G 1 = G Λ := X
A 1 cos Φ
∂Λ =
E 2 sin 2 Φ ) 1 / 2 ( sin Λ E 1 +cos Λ E 2 ) ,
(9.5)
(1
G 2 = G Φ := X
A 1 (1 − E 2 )
∂Φ =
E 2 sin 2 Φ ) 3 / 2 (sin Φ cos Λ E 1 +sin Φ sin Λ E 2 cos Φ E 3 ) .
(9.6)
(1
A 1 denotes the semi-major axis of the e llipsoid-o f-revoluti on, A 2 den otes the semi-minor axis of
the ellipsoid-of-revolution, and E = A 1
A 2 /A 1 = 1
A 2 /A 1 defines the first numerical
eccentricity. The basis vectors finally lead to the elements of the metric tensor.
A 1 cos 2 Φ
E (Gauss) :=
G Λ
|
G Λ
:= G ΛΛ = G 11 =
E 2 sin 2 Φ ,
1
F (Gauss) :=
G Λ |
G Φ
:= G ΛΦ = G 12 = G 21 = G ΦΛ =0 ,
(9.7)
A 1 (1
E 2 ) 2
G (Gauss) :=
G Φ
|
G Φ
:= G ΦΦ = G 22 =
E 2 sin 2 Φ ) 3 .
(1
9-13 The Curvature Tensor of the Ellipsoid-of-Revolution, the Second
Differential Form
Second, let us here compute the second differential form of the surface of type ellipsoid-of-
revolution as follows.
1
H KL = G 3 |∂ 2 X /∂U K ∂U L
=
det[ G KL ] [ G K,L , G 1 , G 2 ] .
(9.8)
The second differential form is related to the determinantal form of the ellipsoid-of-revolution.
We shall compute the surface normal vector G 3 and the surface tangent vectors G 1 and G 2 .
In Box 9.1 , the various steps are collected. Subsequently, we shall collect the coordinates of the
matrix H KL which are derived from the second derivatives, see Box 9.2 . In summary, we present
the coordinates of the curvature tensor of the ellipsoid-of-revolution in ( 9.9 ).
A 1 cos 2 Φ
G 1 /∂U 1
L (Gauss) :=
G 3
|
:= H ΛΛ = H 11 =
E 2 sin 2 Φ ) 1 / 2 ,
(1
G 1 /∂U 2
M (Gauss) :=
G 3 |
:= H ΛΦ = H 12 = H 21 = H ΦΛ =0 ,
(9.9)
E 2 )
A 1 (1
G 2 /∂U 2
N (Gauss) :=
G 3
|
:= H ΦΦ = H 22 =
E 2 sin 2 Φ ) 3 / 2 .
(1
 
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