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P
±'
0
parallel to
equator
P''
0
Fig. 8.14. Curvature of the plumb line along a north-south profile
These quantities ξ, η, ε refer to the earth's surface. Figure 8.13 shows ε .
Similarly, we have for the geoid
ξ 0 0
ϕ,
η 0 =(Λ 0
λ )cos ϕ,
(8-134)
ε 0 = ξ 0 cos α + η 0 sin α. (8-135)
See again Fig. 8.13 for ε 0 , noting that we do not distinguish the normals in
Q 0 and Q 0 as we have mentioned above.
In addition, we need the normal direction of the plumb line at the surface
point P ; it is defined as the tangent to the normal plumb line at P ;the
corresponding latitude and longitude will be denoted by ϕ, λ . In this “local”
notation, there is no danger of confusion with the spherical coordinate ϕ
used in earlier chapters. Hence, we have
λ = λ + δλ normal ,
ϕ = ϕ + δϕ normal ,
(8-136)
where δϕ, δλ express the normal plumb line curvature. These equations are
the “normal equivalent” to (8-131): the “normal surface values” ϕ, λ cor-
respond to the “actual surface values” Φ , Λ and the ellipsoidal values ϕ, λ
correspond to the geoidal values Φ 0 , Λ 0 . To make the analogy complete, we
should replace ϕ = ϕ ( P 0 )by ϕ ( P 0 ), but we have consistently neglected such
differences.
In contrast to the actual plumb line curvature, it is very easy to compute
the normal curvature of the plumb line: from (5-147) we have
0 . 17 h [km] sin 2 ϕ,
δϕ normal =
δλ normal =0 ,
(8-137)
where h [km] denotes elevation in kilometers.
Since the ellipsoidal normal and hence ϕ, λ are geometrically defined, we
may call the quantities (8-132) “geometric deflections of the vertical” at the
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