The processing of the gravity data of the Paris Basin has enlightened
the existence of crustal ridges. These ridges correspond to the zones
of different crustal thicknesses. In plan view, the ridges are concent
ric with the Alpine orogen and were probably controlled by this Tertia
ry Alpine mountain building. The thinned zones related with the Mesozo
ic and pre/Mesozoic basins, were already existing before the Alpine de
formations. These are of limited size and clearly associated with the
basins. On a large scale, two different domains have been recognized.
The first one corresponds with a zone where the crust is 37 km thick.
It is also the place where the Tertiary depocentres developed. The sec
ond one relates with a zone where the crust is 29-30 km thick. It has
been uplifted during the Alpine orogeny. These two observations sugges
t the existence of a Tertiary lithospheric buckling beneath the Paris
Basin.