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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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