The foreland monocline dips underneath thrust belts and accretionary wedges
, both in oceanic and continental subduction zones. We present new data on
the dip of the monocline in the frontal part of two orogens, the Alps and t
he Apennines. There is an overall difference between the dip of the relativ
e monoclines, and there is also a strong lateral variation along both arcs.
In the Alps, the regional dip varies between 0 degrees in the remote forel
and, to an average of 2-3 degrees at the front of the thrust belt below the
foredeep, to about 5 degrees beneath the external thrust-sheets within 40
km from the leading edge of the accretionary wedge. The regional dip of the
monocline in the Apennines has an average of 4-5 degrees at the front of t
he thrust belt below the foredeep, to about 10 degrees beneath the external
thrust-sheets within 40 km from the leading edge of the accretionary wedge
. There are areas where the dip exceeds 20 degrees. The Apennines though to
pographically lower than the Alps present higher monocline dips and a deepe
r foredeep. Moreover, there are variations in the dip of the monocline movi
ng along the strike of the two belts: the low values coincide with Permian-
Mesozoic inherited horsts, whereas the steeper values correspond to basinal
areas, and they usually match the salients of the thrust belt front. Withi
n the salients the distance between thrust ramps increases. Therefore, ther
e are two orders of mean values of the dip of the foreland monocline, the f
irst at the orogen scale (more than 1000 km wavelength), the second at the
regional scale (100-200 km wavelength) within the single orogen. Lateral va
riations in the lithospheric buoyancy due to the inherited Mesozoic stretch
ing may explain the second order variations in foreland dip, but not the fi
rst order mean values which seem to be more sensitive to the geographic pol
arity of the subduction rather than to the lithospheric composition which i
s rather similar in the Alpine and in the central-northern Apennines slabs.
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