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2
þ
2
∂
x
∂
y
G
r
2
ᄐ
∂
l
∂
l
m
2
ᄐ
:
ð
6
:
62
Þ
N
2
cos
2
B
Using the Geodetic Coordinates (B, l ) to Derive the Formula for m
We take the partial derivative with respect to l by applying the formula for the direct
solution of the Gauss projection (
6.28
) to get:
9
=
l
3
∂
x
∂
N
6
sin Bcos
3
B 5
t
2
2
4
l
ᄐ
Nsin Bcos Bl
þ
þ
9
ʷ
þ
4
ʷ
120
sin Bcos
5
B
61
t
4
l
5
N
58t
2
þ
þ
:
ð
6
:
63
Þ
;
l
2
∂
y
∂
N
2
cos
3
B 1
t
2
2
l
ᄐ
N cos B
þ
þʷ
24
cos
5
B
518t
2
2
t
2
l
4
N
t
4
2
þ
þ
þ14ʷ
58ʷ
l
and
∂
y
In (
6.63
), we divide the obtained
∂
x
∂
l
(with the terms containing l
5
and
2
l
3
ʷ
∂
left out) by N cos B; then the square is:
0
@
1
A
2
∂
x
∂
l
l
4
3
sin
2
B cos
2
B 5
l
2
sin
2
B
t
2
N
2
cos
2
B
ᄐ
þ
0
1
2
∂
y
@
A
2
3
2
∂
l
l
2
2
cos
2
B 1
þ
l
4
24
cos
4
B 5
4
5
t
2
2
18t
2
t
4
N
2
cos
2
B
ᄐ
1
þ
þ ʷ
þ
l
4
4
cos
4
B 1
2
l
4
12
cos
4
B 5
l
2
cos
2
B 1
t
2
18t
2
t
4
t
2
2
ᄐ
1
þ
ð
þ ʷ
Þ þ
þ
þ
l
4
3
cos
4
B 2
:
l
2
cos
2
B 1
t
2
2
6t
2
t
4
ᄐ
1
þ
ð
þ ʷ
Þ þ
þ
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