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dividing the terrain by means of a template. Note the difference between
A T , the attraction of the topographic masses, and the terrain correction A t !
Then
= A,
A T
(3-37)
where we now have b = H , c = H P . Use (3-13) with b = H P
for the
innermost circle.
Instead of (3-35), we now have
g B = g
A T + F.
(3-38)
The Bouguer reduction may be still further refined by the consider-
ation of density anomalies, anomalies in the free-air gradient of gravity
(Sect. 2.20), and spherical effects. More computational formulas may be
found in Jung (1961: Sect. 6.4).
3.5
Poincare and Prey reduction
Suppose we need the gravity g inside the earth. Since g cannot be measured,
it must be computed from the surface gravity. This is done by reducing the
measured values of gravity according to the method of Poincar´eandPrey.
We denote the point at which g is to be computed by Q ,sothat g = g Q .
Let P be the corresponding surface point so that P and Q are situated on
the same plumb line (Fig. 3.8). Gravity at P , denoted by g P ,ismeasured.
The direct way of computing g Q would be to use the formula
P
∂g
∂H dH ,
g Q = g P
(3-39)
Q
plumb line
P
Q
H= P
earth's surface
z= Q
geoid
W= 0
P 0
Fig. 3.8. Prey reduction
 
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