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P 0
l
l'
R
r
Q'
Ã
Q
()
dm
r'
(')
dm
Fig. 3.13. Rudzki reduction as an inversion in a sphere
these mass elements at the geoidal point P 0 is
= G dm
l
Gdm
r 2 + R 2
dU T
=
2 Rr cos ψ ,
(3-91)
dU C = G dm
l
Gdm
r 2 + R 2
=
cos ψ .
2 Rr
We should have
dU C = dU T
(3-92)
if
dm = R
r
dm
(3-93)
and
r = R 2
r
.
(3-94)
This is readily verified by substitution into the second equation of (3-91).
The condition (3-94) means that Q and Q are related by inversion in the
sphere of radius R (Kellogg 1929: p. 231). Therefore, this reduction method
is called inversion reduction or Rudzki reduction .
The condition (3-93) expresses the fact that the compensating mass dm
is not exactly equal to dm but is slightly smaller. Since this relative decrease
of mass is of the order of 10 8 , it may be safely neglected by setting
dm = dm .
(3-95)
Usually it is even sucient to replace the sphere by a plane. Then Q is the
ordinary mirror image of Q (Fig. 3.14).
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