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P
l
H
s
dx dy
xy
F
R 2 d
¾
R
R
0
Fig. 6.2. Plane approximation
6.4
Gravity disturbances by upward continuation
We apply Poisson's integral formula (1-123) to the harmonic function T :
T
l 3
= R ( r 2
R 2 )
T P
dσ .
(6-44)
4 π
σ
In the neighborhood of P (Fig. 6.2), the sphere practically coincides with
its tangent plane at F . Since the value of the integrand is very small at
greater distances from P , we may extend the integration over the tangent
plane instead of over the sphere. Then, according to Fig. 6.2,
l = s 2 + H 2 .
(6-45)
We introduce a rectangular coordinate system x, y, z ,the x -axis pointing
north and the y -axis pointing east in the tangent plane. Then we may also
write
l = x 2 + y 2 + H 2 ,
(6-46)
 
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