کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
6430781 1634836 2011 13 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Back-arc rifting initiated with a hot and wet continental lithosphere
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم زمین و سیاره ای (عمومی)
پیش نمایش صفحه اول مقاله
Back-arc rifting initiated with a hot and wet continental lithosphere
چکیده انگلیسی

How back-arc rifting is initiated is studied by inferring the tectonic force and strain rate regimes from published subsidence data for nine back-arc basins in the European Tethyan belt and in the western Pacific. The results show that rifting only begins after some particular magnitude of tectonic force is reached. This implies that subduction has already progressed to a point such that the total negative buoyancy of the slab becomes so large that the relevant tectonic force exceeds its bending strength. Once back-arc rifting has been initiated, the force required to maintain it gradually decays. This indicates that the processes governing back-arc extension are fast enough that lithosphere weakening due to an increase in geothermal gradient exceeds strengthening due to the thermal relaxation and crustal thinning. This is achieved, given currently accepted estimates for the maximum force (≤ 7 TN/m), if the thickness of the thermal lithosphere is significantly less than 125 km and if the lithosphere has a wet rheology, meaning that a weak continental lithosphere is required for the initiation of back-arc rifting. The presence of significant strength in the uppermost mantle is not precluded, but it is not required.

Research Highlights► Back-arc rifting is highly favoured by a hot and wet continental lithosphere, inferred from inverting tectonic subsidence data in Tethyan and western Pacific basins. ► Back-arc rifting begins only some time after the onset of subduction: this allows the force derived from the negative buoyancy of the subducted slab to build-up but is also important for promoting the weakening of the over-riding lithosphere, by heating and hydration.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Earth and Planetary Science Letters - Volume 302, Issues 1–2, 1 February 2011, Pages 172-184
نویسندگان
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