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    Unraveling the geometry of the New England oroclines (eastern Australia): Constraints from magnetic fabrics

    225268_140585_Tectonics_Serg.pdf (14.08Mb)
    Access Status
    Open access
    Authors
    Mochales, T.
    Rosenbaum, G.
    Speranza, F.
    Pisarevskiy, Sergei
    Date
    2014
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Mochales, T. and Rosenbaum, G. and Speranza, F. and Pisarevskiy, S. 2014. Unraveling the geometry of the New England oroclines (eastern Australia): Constraints from magnetic fabrics. Tectonics. 33 (11): pp. 2261-2282.
    Source Title
    Tectonics
    DOI
    10.1002/2013TC003483
    ISSN
    0278-7407
    School
    Department of Applied Geology
    Remarks

    An edited version of this paper was published by AGU. Copyright 2014 American Geophysical Union

    URI
    http://hdl.handle.net/20.500.11937/5651
    Collection
    • Curtin Research Publications
    Abstract

    The 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 historywith respect to the rest of the NEO.

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