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  5. Crustal structure in the Southern Apennines from teleseismic receiver functions
 
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Crustal structure in the Southern Apennines from teleseismic receiver functions

Author(s)
Steckler, M. S.  
Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York  
Piana Agostinetti, N.  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia  
Wilson, C. K.  
Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York  
Roselli, P.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia  
Seeber, L.  
Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York  
Amato, A.  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia  
Lerner-Lam, A.  
Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York  
Language
English
Obiettivo Specifico
3.3. Geodinamica e struttura dell'interno della Terra
Status
Published
JCR Journal
JCR Journal
Journal
Geology  
Issue/vol(year)
2/36 (2008)
Publisher
Geological Society of America
Pages (printed)
155-158
Date Issued
February 2008
DOI
10.1130/G24065A.1
Last version
http://hdl.handle.net/2122/3309
URI
https://www.earth-prints.org/handle/2122/4545
Subjects
01. Atmosphere::01.03. Magnetosphere::01.03.04. Structure and dynamics  
Subjects

thrust tectonics

Apennines

continental collision...

seismology

receiver functions

structural geology

Abstract
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. Inter-
pretation 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.
Type
article
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