Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/4545
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dc.contributor.authorallSteckler, M. S.; Lamont-Doherty Earth Observatory of Columbia University, Palisades, New Yorken
dc.contributor.authorallPiana Agostinetti, N.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italiaen
dc.contributor.authorallWilson, C. K.; Lamont-Doherty Earth Observatory of Columbia University, Palisades, New Yorken
dc.contributor.authorallRoselli, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.authorallSeeber, L.; Lamont-Doherty Earth Observatory of Columbia University, Palisades, New Yorken
dc.contributor.authorallAmato, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione CNT, Roma, Italiaen
dc.contributor.authorallLerner-Lam, A.; Lamont-Doherty Earth Observatory of Columbia University, Palisades, New Yorken
dc.date.accessioned2008-12-09T14:47:13Zen
dc.date.available2008-12-09T14:47:13Zen
dc.date.issued2008-02en
dc.identifier.urihttp://hdl.handle.net/2122/4545en
dc.description.abstractWhile 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.en
dc.language.isoEnglishen
dc.publisher.nameGeological Society of Americaen
dc.relation.ispartofGeologyen
dc.relation.ispartofseries2/36 (2008)en
dc.relation.isversionofhttp://hdl.handle.net/2122/3309en
dc.subjectthrust tectonicsen
dc.subjectApenninesen
dc.subjectcontinental collisionen
dc.subjectseismologyen
dc.subjectreceiver functionsen
dc.subjectstructural geologyen
dc.titleCrustal structure in the Southern Apennines from teleseismic receiver functionsen
dc.typearticleen
dc.description.statusPublisheden
dc.description.pagenumber155-158en
dc.subject.INGV01. Atmosphere::01.03. Magnetosphere::01.03.04. Structure and dynamicsen
dc.identifier.doi10.1130/G24065A.1en
dc.description.obiettivoSpecifico3.3. Geodinamica e struttura dell'interno della Terraen
dc.description.journalTypeJCR Journalen
dc.description.fulltextreserveden
dc.contributor.authorSteckler, M. S.en
dc.contributor.authorPiana Agostinetti, N.en
dc.contributor.authorWilson, C. K.en
dc.contributor.authorRoselli, P.en
dc.contributor.authorSeeber, L.en
dc.contributor.authorAmato, A.en
dc.contributor.authorLerner-Lam, A.en
dc.contributor.departmentLamont-Doherty Earth Observatory of Columbia University, Palisades, New Yorken
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italiaen
dc.contributor.departmentLamont-Doherty Earth Observatory of Columbia University, Palisades, New Yorken
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italiaen
dc.contributor.departmentLamont-Doherty Earth Observatory of Columbia University, Palisades, New Yorken
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italiaen
dc.contributor.departmentLamont-Doherty Earth Observatory of Columbia University, Palisades, New Yorken
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptLamont-Doherty Observatory, Palisades, NY (USA)-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia-
crisitem.author.deptLamont-Doherty Earth Observatory of Columbia University-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptColumbia University-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione ONT, Roma, Italia-
crisitem.author.deptLamont-Doherty Earth Observatory of Columbia University-
crisitem.author.orcid0000-0003-3844-5059-
crisitem.author.orcid0000-0002-9521-6570-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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