کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
6428383 1634739 2015 10 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Spin state transition and partitioning of iron: Effects on mantle dynamics
ترجمه فارسی عنوان
انتقال اسپین حالت و پراکندگی آهن: تأثیر روی پویایی گوشته
کلمات کلیدی
انتقال اسپین حالت، گوساله پایین تر زمین، جداسازی آهن، همرفت، ژئودینامیک،
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم زمین و سیاره ای (عمومی)
چکیده انگلیسی


- We model the effect of Fe2+ spin state transition in Ferropericlase on density.
- We study two pyrolitic compositions, an Al-bearing and an Al-free.
- We consider Fe partitioning between ferropericlase and perovskite.
- We include the calculated density profile in the convection code Stag3D.
- We find significant consequences on plumes and slabs flow velocity.

Experimental studies at pressure and temperature conditions of the Earth's lower mantle have shown that iron in ferropericlase (Fp) and in Mg-silicate perovskite (Pv) undergoes a spin state transition. This electronic transition changes elastic and transport properties of lower mantle minerals and can play an important role in mantle convection. Here we focus on the geodynamic effect of the spin-induced density modifications caused by the volume collapse of Fp and by the variation of Fe partitioning (KPv-Fp) between Fp and Pv. Since KPv-Fp behavior strongly depends on alumina content, we explore two end-member compositions, one Al-bearing (with 4.7 wt% Al2O3 in Pv) and the other Al-free. We use the theoretical model by Sturhahn et al. (2005) to calculate the spin configuration of Fp over a range of pressure-temperature conditions, and use experimental results to model Fe partitioning. We then apply the Mie-Grüneisen-Debye equation of state to obtain the density of the mineral assemblages. The calculated amplitude of the density change across the spin state transition is less than 1%, consistent with experiments by Mao et al. (2011); our density profiles differ from PREM by less than 1.5%. The spin-induced density variations are included in a three dimensional convection code (Stag3D) for a compressible mantle. We find small temperature differences between models with and without spin state transitions, since over billions of years the relative temperature difference is less than 50 K. However the relative RMS vertical velocity difference is up to 15% for an Al-free system, but only less than 6% for an Al-bearing system.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Earth and Planetary Science Letters - Volume 417, 1 May 2015, Pages 57-66
نویسندگان
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