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Geology; February, 2008; v. 36; no. 2; p. 155-158; DOI: 10.1130/G24065A.1
© 2008 Geological Society of America
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Crustal structure in the Southern Apennines from teleseismic receiver functions

Michael S. Steckler1, Nicola Piana Agostinetti2, Charles K. Wilson3, Pamela Roselli4, Leonardo Seeber5, Alessandro Amato6 and Arthur Lerner-Lam7

1 Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York 10964, USA
2 Istituto Nazionale di Geofisica e Vulcanologica, Centro Nazionale Terremoti, 00143 Rome, Italy
3 Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York 10964, USA
4 Istituto Nazionale di Geofisica e Vulcanologica, Osservatorio Sismologico Arezzo, 52100 Arezzo, Italy
5 Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York 10964, USA
6 Istituto Nazionale di Geofisica e Vulcanologica, Centro Nazionale Terremoti, 00143 Rome, Italy
7 Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York 10964, USA

While the upper crustal structure of the Southern Apennines is known, lack of control on the deep structure allows competing thin-skinned and thick-skinned models of the orogen. In thin-skinned models, the detachment decouples a stack of rootless nappes from the basement. In thick-skinned models, basement is involved in the most recent phase of thrusting. To examine crustal structure, we use teleseismic data from the Calabria-Apennine-Tyrrhenian/Subduction-Accretion-Collision Network (CAT/SCAN) array in southern Italy. We use receiver functions (RF) processed into a common conversion point stack to generate images of the crust. Interpretation and correlation to geological structure are done using inversions of individual station RFs. We focus on a shallow discontinuity where P-to-S conversions occur. In the foreland, it corresponds to velocity jumps between carbonate and clastic strata with basement. A similar interpretation for the Apennines provides the most parsimonious explanation and supports a thick-skinned interpretation. In a thick-skinned reconstruction, the amount of shortening is much smaller than for a thin-skinned model. This implies considerably less Pliocene–Pleistocene shortening across the Apennines and suggests an east-southeast motion of the Calabrian arc subparallel to the southern Apennines rather than a radial expansion of the arc.

Key Words: thrust tectonics • Apennines • continental collision • seismology • receiver functions • structural geology




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