Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9162
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dc.contributor.authorallMochales, T.; School of Earth Sciences, University of Queensland, Brisbane, Queensland, Australiaen
dc.contributor.authorallRosenbaum, G.; School of Earth Sciences, University of Queensland, Brisbane, Queensland, Australiaen
dc.contributor.authorallSperanza, F.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallPisarevsky, S. A.; School of Earth and Environment, University of Western Australia, Crawley, Western Australiaen
dc.date.accessioned2014-12-04T09:48:16Zen
dc.date.available2014-12-04T09:48:16Zen
dc.date.issued2014-10-16en
dc.identifier.urihttp://hdl.handle.net/2122/9162en
dc.description.abstractThe southern New England Orogen (NEO) in eastern Australia is characterized by tight curvatures (oroclines), but the exact geometry of the oroclines and their kinematic evolution are controversial. Here we present new data on the anisotropy ofmagnetic susceptibility (AMS), which provide a petrofabric proxy for the finite strain associated with the oroclines. We focus on a series of preoroclinal Devonian-Carboniferous fore-arc basin rocks, which are aligned parallel to the oroclinal structure, and by examining structural domains, we test whether or not the magnetic fabric is consistent with the strain axes. AMS data show a first-order consistency with the shape of the oroclines, characterized, in most of structural domains, by subparallelism between magnetic lineations, “structural axis” and bedding. With the exception of the Gresford and west Hastings domains, our results are relatively consistent with the existence of the Manning and Nambucca (Hastings) Oroclines. Reconstruction of magnetic lineations to a prerotation (i.e., pre–late Carboniferous) stage, considering available paleomagnetic results, yields a consistent and rather rectilinear NE-SW predeformation fore-arc basin. This supports the validity of AMS as a strain proxy in complex orogens, such as the NEO. In the Hastings Block, magnetic lineations are suborthogonal to bedding, possibly indicating a different deformational history with respect to the rest of the NEO.en
dc.language.isoEnglishen
dc.publisher.nameAmerican Geophysical Unionen
dc.relation.ispartofTectonicsen
dc.relation.ispartofseries/33 (2014)en
dc.subjectAMS data, magnetic fabric, oroclinesen
dc.titleUnraveling the geometry of the New England oroclines (eastern Australia): Constraints from magnetic fabricsen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber2261–2282en
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.06. Paleomagnetismen
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.01. Continentsen
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.05. Stressen
dc.subject.INGV04. Solid Earth::04.07. Tectonophysics::04.07.07. Tectonicsen
dc.identifier.doi10.1002/2013TC003483en
dc.description.obiettivoSpecifico1A. Geomagnetismo e Paleomagnetismoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0278-7407en
dc.relation.eissn1944-9194en
dc.contributor.authorMochales, T.en
dc.contributor.authorRosenbaum, G.en
dc.contributor.authorSperanza, F.en
dc.contributor.authorPisarevsky, S. A.en
dc.contributor.departmentSchool of Earth Sciences, University of Queensland, Brisbane, Queensland, Australiaen
dc.contributor.departmentSchool of Earth Sciences, University of Queensland, Brisbane, Queensland, Australiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentSchool of Earth and Environment, University of Western Australia, Crawley, Western Australiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptInstituto Geológico y Minero de España, Madrid, España-
crisitem.author.deptSchool of Physical Sciences, University of Queensland, Brisbane, Queensland 4072, Australia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptSchool of Earth and Environment, University of Western Australia, Crawley, Western Australia-
crisitem.author.orcid0000-0001-5492-8670-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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