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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Volumetric changes in weathered profiles: iso-element mass balance method questioned by magnetic fabric
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Volumetric changes in weathered profiles: iso-element mass balance method questioned by magnetic fabric

机译:风化剖面的体积变化:磁性织物质疑等元素质量平衡方法

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A major issue in understanding weathering processes is to determine to what extent fabrics, structures and volumes from the parent rock are preserved through the weathering profile. Iso-element mass balance methods (IMB) are often used to estimate volume changes during progressive weathering, based on the assumption that a given element (either Ti, Zr or Th) is not mobile. The petrofabric of the weathered material is often characterized by a mimetic replacement of primary minerals that fully preserve the primary fabric. This suggests an isovolume weathering as volume change must be associated with shape change due to boundary conditions not allowing horizontal strains. So collapse or dilation should induce vertical compaction or constriction, respectively. The weak petrofabric of weathered materials may be precisely quantified using the anisotropy of low-field magnetic susceptibility technique (AMS). This paper reports, for the first time, a combined IMB and AMS study of two different environments: a complex lateritic sequence on Precambrian metamorphic rocks in Cameroon and a weathering profile on a Pleistocene basaltic flow in Morocco. The lateritic profile, divided into a lower saprolite zone (> 12 m) and an upper nodular iron-rich unit (4 m), is characterized by neoformed magnetic minerals (goethite/hematite/spinels) and a weak but rather consistent magnetic fabric. Saprolitization, which induces low susceptibility values (50 * 10~(-9) m~3/kg), preserves the linear tectonic fabric of the parent gneiss. AMS evidence for isovolumetric weathering agrees with Th based IMB, while Ti and Zr partly indicate apparent collapse and dilation (up to 50%), respectively. Ferralitization in the nodular iron crust, which enhances susceptibilities (500 to 700 * 10~(-9) m~3/kg, due to spinel phases), induces drastic reductions in anisotropy due to multiple generation of neoformed minerals destroying primary fabric. However, a weak horizontal planar magnetic fabric suggests compaction, in agreement with Th and Ti based IMB while Zr would indicate isovolume weathering. Conversely, in the one meter thick weathering profile on basalt, the strong susceptibility (1.5 to 3 * 10~(-6) m~3/kg) is dominated by inherited titanomaghemite grains which totally preserve the weak magmatic fabric of the fresh basalt. This again suggests that volume change is minor, while Ti and Zr based IMB indicate 20 to 50% of dilation. In both examples, large volume changes inferred from the IMB in units showing preserved primary AMS fabric appear unrealistic. Our AMS study, together with the large discrepancies between the IMB results produced by various elements, indicate that the assumption of immobility of a given element is probably not fulfil
机译:理解风化过程的主要问题是确定通过风化剖面将母岩的织物,结构和体积保存到何种程度。基于给定元素(Ti,Zr或Th)不可移动的假设,等元素质量平衡方法(IMB)通常用于估算渐进风化过程中的体积变化。风化材料的石油织物通常以模拟替代主要矿物的特征为特征,该矿物完全保留了主要织物。这表明等体积风化,因为边界条件不允许水平应变,体积变化必须与形状变化相关联。因此,塌陷或膨胀应分别引起垂直压实或收缩。可以使用低场磁化率技术(AMS)的各向异性来精确定量风化材料的弱石油织物。本文首次报道了结合IMB和AMS的两种不同环境研究:喀麦隆前寒武纪变质岩上复杂的红土层序和摩洛哥更新世玄武岩流上的风化剖面。红土剖面分为下部的腐泥土带(> 12 m)和上部的球状富铁单元(4 m),其特征是新形成的磁性矿物(针铁矿/赤铁矿/尖晶石)和薄弱但稳定的磁性织物。腐泥土的磁化率低(50 * 10〜(-9)m〜3 / kg),可以保留亲片麻岩的线性构造构造。等容风化的AMS证据与基于Th的IMB一致,而Ti和Zr分别部分表明明显的塌陷和膨胀(高达50%)。球状铁皮中的铁素体化提高了磁化率(由于尖晶石相而使磁化率提高到500至700 * 10〜(-9)m〜3 / kg / kg),由于新生成的矿物的多次破坏破坏了初级织物,导致各向异性大大降低。然而,与基于Th和Ti的IMB一致,较弱的水平平面磁性织物建议压实,而Zr则表明等体积风化。相反,在玄武岩上一米厚的风化剖面中,强烈的磁化率(1.5至3 * 10〜(-6)m〜3 / kg)由继承的钛磁赤铁矿晶粒占据,这完全保留了新鲜玄武岩的弱岩浆构造。这再次表明体积变化很小,而基于Ti和Zr的IMB则表明有20%到50%的膨胀。在两个示例中,从IMB推断出的大量更改(以显示保留的主要AMS结构为单位)似乎都是不现实的。我们的AMS研究以及各种要素产生的IMB结果之间的巨大差异,表明给定要素的固定性假设可能无法满足

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