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Integrating this relation yields the difference of the height anomaly
B
B
g
γ
ζ B
ζ A =
εds
dh ;
(8-150)
A
A
the gravity anomaly ∆ g refers to the earth's surface according to (8-128).
The first term on the right-hand side represents the Helmert integral (8-143)
of the surface deflection ε , and the second term is Molodensky's correction to
the Helmert integral, necessary to obtain height anomalies. This correction
depends on the gravity g at the earth's surface.
8.14
Topographic-isostatic reduction of vertical
deflections
For the reasons mentioned at the end of the preceding section, it is nat-
ural to try and find a way which makes use of the clear advantages of the
topographic-isostatic reduction but avoids the problems inherent in a free-air
reduction from the surface point P to the geoidal point P 0 .
In Sect. 8.9, we have treated the reduction of gravity from the modern
point of view. The second formula of (8-95) is
g c = g − δg .
(8-151)
Everything is referred to the ground point P ,and δg = δg TI is the effect
of gravity reduction on g ,alsoat P .Inthe topographic-isostatic reduction
which we use here exclusively , it is the gravitational attraction of the to-
pography minus the gravitational attraction of the compensating isostatic
masses, topography minus isostasy.
To get the topographic-isostatic gravity anomaly, we subtract normal
gravity γ , also referred to ground level, more precisely, to the corresponding
telluroid point Q .Thus,
g c =∆ g
δg TI .
(8-152)
The explanation is trivial: you are standing at point P and watch how the
topography is removed to fill the isostatic mass deficits, but by a miracle
you are still hovering at P , now in “free air”.
Application to deflections of the vertical
The gravity anomaly is only one component of the anomalous gravity vector,
the other two being the vertical components ξ and η , both, of course, mul-
tiplied by γ to get the dimensions right. Thus, ξ and η can be isostatically
reduced in exactly the same way.
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