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are the equations of the geoid and the ellipsoid, where in general the con-
stants W 0 and U 0 are different. As in Sect. 2.12, we have, using Fig. 2.12,
W P
= U Q
γN + T , but now U Q = U 0
= W 0 = W P ,sothat
γN = T
( W 0
U 0 ) .
(2-345)
Denoting the difference between the potentials by
δW = W 0 − U 0 ,
(2-346)
we obtain the following simple generalization of Bruns' formula:
N = T
δW
γ
.
(2-347)
We also need the extension of Eqs. (2-246) through (2-250). Those for-
mulas which contain N instead of T are easily seen to hold for an arbitrary
reference ellipsoid as well, but the transition from N to T is now effected by
means of (2-347). Hence, Eq. (2-247), i.e.,
∂T
∂h + ∂γ
g =
∂h N,
(2-348)
remains unchanged, but (2-248) becomes
∂T
∂h + 1
∂γ
∂h T
1
γ
∂γ
∂h δW .
g =
(2-349)
γ
Therefore, the fundamental boundary condition is now
∂T
∂γ
∂γ
∂h δW .
∂h + 1
∂h T =∆ g + 1
(2-350)
γ
γ
The spherical approximations of these equations are
N = T
δW
γ 0
(2-351)
and
∂T
∂r
2
R T +
2
R δW
g =
(2-352)
and
∂T
∂r
2
R T =∆ g
2
R δW .
(2-353)
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