New gravity maps of the Eastern Alps and significance for the crustal structures

Autor(en)
Claudio Zanolla, Carla Braitenberg, Jörg Ebbing, Marcello Bernabini, Kurt Bram, Gerald Gabriel, Hans J. Götze, Salvatore Giammetti, Bruno Meurers, Rinaldo Nicolich, Franco Palmieri
Abstrakt

The deep seismic profile T ransalp crosses, from north to south, Germany, Austria and Italy. The gravity measurements for each country were made by national agencies with different reference systems and data reduction methods. Within the frame of the TRANSALP-project a comprehensive database of the Eastern Alps was compiled covering an area of 3.5° by 4° in longitude and latitude (275 by 445 km), respectively. To increase the data coverage in the south Alpine area two gravity surveys were carried out, resulting in 469 areally distributed new stations, of which 215 have been measured with the intent to improve the geoid in the area of the planned Brenner Basistunnel (BBT). The resulting gravity database is the best in terms of resolution and data quality presently available for the Eastern Alps. Here the free air, Bouguer and isostatic gravity fields are critically discussed. The spatial density of existing gravity stations in the three countries is discussed. On the Italian side of the Alps the spatial density is rather sparse compared to the Austrian side. The Bouguer-gravity field varies between - 190* 10-5 m/s2 and +25* 10-5 m/s2, with the minimum located along the Alpine high topographic chain, but with a small offset (a few tens of km) to the greatest topographic elevation, showing that the Airy-type local isostatic equilibrium does not fully apply here. The maximum of the Bouguer anomaly has an elongated shape of 100 by 50 km located between the towns of Verona and Vicenza and covers the Venetian Tertiary Volcanic Province (VTVP), a feature not directly related to the plate collision in the Eastern Alps. The gravity high is only partly explainable by high-density magmatic rocks and requires also a deeper source, like a shallowing of the Moho. The isostatic residual anomalies (Airy model) are in the range ‘ 50* 10-5 m/s2, with the greatest positive anomaly corresponding to the location of the VTVP, indicating here under-compensation of masses. At last a discussion of a 2D density model based on reflection seismic data and receiver functions is made. Œ 2005 Elsevier B.V. All rights reserved.

Organisation(en)
Institut für Meteorologie und Geophysik
Externe Organisation(en)
Istituto Nazionale di Oceanografia e di Geofisica Sperimentale, Università degli Studi di Trieste, Geological Survey of Norway, Università degli Studi di Roma La Sapienza, Institut für Geowissenschaftliche Gemeinschaftsaufgaben, Christian-Albrechts-Universität zu Kiel, Eni S.p.A.
Journal
Tectonophysics
Band
414
Seiten
127-143
Anzahl der Seiten
17
ISSN
0040-1951
Publikationsdatum
2006
Peer-reviewed
Ja
ÖFOS 2012
105102 Allgemeine Geophysik
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/ab3b2cdc-cd00-44c8-9755-62807ceaca57