Oblique rifting: the rule, not the exception

Movements of tectonic plates often induce oblique deformation at divergent plate boundaries. This is in striking contrast with traditional conceptual models of rifting and rifted margin formation, which often assume 2-D deformation where the rift velocity is oriented perpendicular to the plate bound...

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Published in:Solid Earth
Main Authors: Brune, Sascha, Williams, Simon E., Müller, R. Dietmar
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2018
Subjects:
Online Access:https://doi.org/10.5194/se-9-1187-2018
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spelling ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00004263 2023-05-15T13:34:49+02:00 Oblique rifting: the rule, not the exception Brune, Sascha Williams, Simon E. Müller, R. Dietmar 2018-10 electronic https://doi.org/10.5194/se-9-1187-2018 https://noa.gwlb.de/receive/cop_mods_00004263 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00004220/se-9-1187-2018.pdf https://se.copernicus.org/articles/9/1187/2018/se-9-1187-2018.pdf eng eng Copernicus Publications Solid Earth -- 1869-9529 https://doi.org/10.5194/se-9-1187-2018 https://noa.gwlb.de/receive/cop_mods_00004263 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00004220/se-9-1187-2018.pdf https://se.copernicus.org/articles/9/1187/2018/se-9-1187-2018.pdf https://creativecommons.org/licenses/by/4.0/ uneingeschränkt info:eu-repo/semantics/openAccess CC-BY article Verlagsveröffentlichung article Text doc-type:article 2018 ftnonlinearchiv https://doi.org/10.5194/se-9-1187-2018 2022-02-08T23:00:12Z Movements of tectonic plates often induce oblique deformation at divergent plate boundaries. This is in striking contrast with traditional conceptual models of rifting and rifted margin formation, which often assume 2-D deformation where the rift velocity is oriented perpendicular to the plate boundary. Here we quantify the validity of this assumption by analysing the kinematics of major continent-scale rift systems in a global plate tectonic reconstruction from the onset of Pangea breakup until the present day. We evaluate rift obliquity by joint examination of relative extension velocity and local rift trend using the script-based plate reconstruction software pyGPlates. Our results show that the global mean rift obliquity since 230 Ma amounts to 34° with a standard deviation of 24°, using the convention that the angle of obliquity is spanned by extension direction and rift trend normal. We find that more than ∼ 70 % of all rift segments exceeded an obliquity of 20° demonstrating that oblique rifting should be considered the rule, not the exception. In many cases, rift obliquity and extension velocity increase during rift evolution (e.g. Australia-Antarctica, Gulf of California, South Atlantic, India-Antarctica), which suggests an underlying geodynamic correlation via obliquity-dependent rift strength. Oblique rifting produces 3-D stress and strain fields that cannot be accounted for in simplified 2-D plane strain analysis. We therefore highlight the importance of 3-D approaches in modelling, surveying, and interpretation of most rift segments on Earth where oblique rifting is the dominant mode of deformation. Article in Journal/Newspaper Antarc* Antarctica Niedersächsisches Online-Archiv NOA Solid Earth 9 5 1187 1206
institution Open Polar
collection Niedersächsisches Online-Archiv NOA
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language English
topic article
Verlagsveröffentlichung
spellingShingle article
Verlagsveröffentlichung
Brune, Sascha
Williams, Simon E.
Müller, R. Dietmar
Oblique rifting: the rule, not the exception
topic_facet article
Verlagsveröffentlichung
description Movements of tectonic plates often induce oblique deformation at divergent plate boundaries. This is in striking contrast with traditional conceptual models of rifting and rifted margin formation, which often assume 2-D deformation where the rift velocity is oriented perpendicular to the plate boundary. Here we quantify the validity of this assumption by analysing the kinematics of major continent-scale rift systems in a global plate tectonic reconstruction from the onset of Pangea breakup until the present day. We evaluate rift obliquity by joint examination of relative extension velocity and local rift trend using the script-based plate reconstruction software pyGPlates. Our results show that the global mean rift obliquity since 230 Ma amounts to 34° with a standard deviation of 24°, using the convention that the angle of obliquity is spanned by extension direction and rift trend normal. We find that more than ∼ 70 % of all rift segments exceeded an obliquity of 20° demonstrating that oblique rifting should be considered the rule, not the exception. In many cases, rift obliquity and extension velocity increase during rift evolution (e.g. Australia-Antarctica, Gulf of California, South Atlantic, India-Antarctica), which suggests an underlying geodynamic correlation via obliquity-dependent rift strength. Oblique rifting produces 3-D stress and strain fields that cannot be accounted for in simplified 2-D plane strain analysis. We therefore highlight the importance of 3-D approaches in modelling, surveying, and interpretation of most rift segments on Earth where oblique rifting is the dominant mode of deformation.
format Article in Journal/Newspaper
author Brune, Sascha
Williams, Simon E.
Müller, R. Dietmar
author_facet Brune, Sascha
Williams, Simon E.
Müller, R. Dietmar
author_sort Brune, Sascha
title Oblique rifting: the rule, not the exception
title_short Oblique rifting: the rule, not the exception
title_full Oblique rifting: the rule, not the exception
title_fullStr Oblique rifting: the rule, not the exception
title_full_unstemmed Oblique rifting: the rule, not the exception
title_sort oblique rifting: the rule, not the exception
publisher Copernicus Publications
publishDate 2018
url https://doi.org/10.5194/se-9-1187-2018
https://noa.gwlb.de/receive/cop_mods_00004263
https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00004220/se-9-1187-2018.pdf
https://se.copernicus.org/articles/9/1187/2018/se-9-1187-2018.pdf
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op_relation Solid Earth -- 1869-9529
https://doi.org/10.5194/se-9-1187-2018
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https://se.copernicus.org/articles/9/1187/2018/se-9-1187-2018.pdf
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