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8.1.4 Attraction of the Compensating Masses

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8.1 CLASSICAL ISOSTATIC MODELS

229 To repeat, this extremely simple solution is not the equation of the actual ben- ding curve (8-20) but gives an excel1ent qualitative picture. This can be seen by drawing the graph of (8-27), with x replaced by -x for negative values of x: a central depression surrounded by very small waves of decreasing amplitude.

8.1.4 Attraction of the Compensating Masses

As apreparatory step for computing isostatic reductions, to be discussed in sec. 8.1.5, we need the attraction of the compensating masses. For simplicity we consider the problem in the usuallocal plane approximation, replacing the geoid by its tangential plane. The spherical approximation will be used later (sec. 8.2).

We shall assume a basic definition concerning our three-dimensionallocal Carte- sian co ordinate system (Fig. 8.6): The xy-plane represents sea level, the z-axis points

h

p

--~---~L---~~----,---~xy

o

z dv

z

FIGURE 8.6: The basic co ordinate systems xyz and xyh

vertically downwardJ, whereas the h-axis points vertically upward3, so that, for an arbitrary point,

z =-h (8-28)

Keeping this definition in mind, the distance I between the computation point P and the volume element dv becomes

(8-29)

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