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Fig. 5.32 Correction for
skew normals
N
2
e
2
sin B
2
N
1
e
2
sin B
1
N
2
e
2
K
a
K
b
ᄐ
OK
b
OK
a
ᄐ
ð
sin B
2
sin B
1
Þ
,
S
cos A
1
M
1
With the differential equation of geodesics B
2
B
1
þ
, one obtains:
N
2
e
2
cos B
1
S cos A
1
M
1
K
a
K
b
ᄐ
:
Inserting back into the above equation and rearranging gives:
e
2
H
2
ˁ
00
cos
2
B
2
sin 2A
1
,
ʴ
2
ᄐ
ð
5
:
56
Þ
2M
2
where B
2
and M
2
are the geodetic latitude and meridian radius of curvature of the
target point, A
1
is the geodetic azimuth of the observed direction, and H
2
is the
height of the target (actual target point in observation) relative to the ellipsoid,
consisting of three parts:
H
2
ᄐ
H
2N
þ ʶ
2
þ
a
2
,
where H
2N
is the normal height of the monument center of target point,
ʶ
2
is the
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