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Fig. 14.7 Mechanism of isostatic compensation. Starting
from a hypothetical initial situation where the elevation
is zero everywhere, a lateral increase of crustal thickness
in the continental crust ( green regions , density ¡ c ) will
determine upward motion to compensate the decreased
weight of the column. Similarly, the denser oceanic crust
( ¡ o > ¡ c ) will subside to compensate the excess weight
with water ( blue regions , density ¡ w ). In this example,
the lithospheric mantle has constant thickness and density
¡ l > ¡ c , ¡ o .Theair( yellow regions ) has negligible density.
Finally, it is assumed that the asthenosphere has density
¡ a l
Fig. 14.8 Geoid anomalies, N , and dynamic topography
of a fluid mantle layer that incorporates small density
anomalies. The geoid undulations result ( thick solid line )
from the combined effect of static density contrasts ( thin
solid line ) and topography variations ( dashed lines )at
the upper and lower boundaries of the layer induced by
mantle flows ( dotted lines )
However, in some regions the elevated or
depressed topography cannot be explained in
terms of isostasy. A classic example is given by
the East African and Ethiopian plateaux (Moucha
and Forte 2011 ). Hager ( 1984 ) and Richards
and Hager ( 1984 ) were the first to propose
a mechanism that today is known as dynamic
topography .
The basic idea behind the concept of dynamic
topography is illustrated in Fig. 14.8 .Itstarts
from the simple observation that mantle con-
vection should cause deformation and topogra-
phy variations at the Earth's surface. In fact,
sinking density anomalies pull downwards man-
tle material located above them. At the same
time, they push the mantle downwards at their
front. Similarly, a rising density contrast pulls
or pushes mantle material upwards. Both these
situations determine flexure of the upper man-
tle boundaries and surface topography changes.
The same mechanism would cause variations
in the topography of the CMB associated with
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