|
|||||
|
|
Geophysical Study of the Valle Fértil Lineament Between 28°45′S and 31°30′S: Boundary Between the Cuyania and Pampia Terranes |
|
| Authors: | Antonio Introcaso Myriam P Martínez Mario E Gimnez Francisco Ruiz |
| Institution: | aInstituto de Física Rosario Universidad Nacional de Rosario and CONICET, Av. Pellegrini 250, 2000 Rosario, Argentina bInstituto Geofísico Sismológico Ing. Fernando S. Volponi Universidad Nacional de San Juan, Avda. Ignacio de la Roza y Meglioli, Rivadavia, 5400 San Juan, Argentina |
| Abstract: | A gravimetric and magnetometric study was carried out in the north-eastern portion of the Cuyania terrane and adjacent Pampia terrane. Gravimetric models permitted to interpret the occurrence of dense materials at the suture zone between the latter terranes. Magnetometric models led to propose the existence of different susceptibilities on either side of the suture. The Curie temperature point depth, representing the lower boundary of the magnetised crust, was found to be located at 25 km, consistent with the lower limit of the brittle crust delineated by seismic data; this unusually thick portion of the crust is thought to release stress producing significant seismicity. Moho depths determined from seismic studies near western Sierras Pampeanas are significantly greater than those obtained from gravimetric crustal models. Considering mass and gravity changes originated by the flat-slab Nazca plate along Cuyania and western Pampia terranes, it is possible to reconcile Moho thickness obtained either by seismic or by gravity data. Thus, topography and crustal thickness are controlled not only by erosion and shortening but by upper mantle heterogeneities produced by: (a) the oceanic subducted Nazca plate with “normal slope” also including asthenospheric materials between both continental and oceanic lithospheres; (b) flat-slab subducted Nazca plate (as shown in this work) without significant asthenospheric materials between both lithospheres. These changes influence the relationship between topographic altitudes and crustal thickness in different ways, differing from the simple Airy system relationship and modifying the crustal scale shortening calculation. These changes are significantly enlarged in the study area. Future changes in Nazca Plate slope will produce changes in the isostatic balance. |
| Keywords: | Gravity magnetometry Valle Fértil lineament Cuyania-Pampia terranes isostasy |
| 本文献已被 ScienceDirect 等数据库收录！ | |