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首页> 外文期刊>Quaternary International >Climatic control of magnetic granulometry in the Mircea Voda loess/paleosol sequence (Dobrogea, Romania)
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Climatic control of magnetic granulometry in the Mircea Voda loess/paleosol sequence (Dobrogea, Romania)

机译:Mircea Voda黄土/古土壤序列中磁粒度仪的气候控制(罗马尼亚多布罗加)

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摘要

A detailed rock-magnetic investigation of loess/palaeosol samples from the section at Mircea Voda (Dobrogea Plateau, Romania) is presented. Investigation of climatic control on magnetic granulometry used several grain-size and concentration-dependent proxies (magnetic susceptibility and its frequency dependence, anhysteretic remanent magnetization, isothermal remanent magnetization, hysteresis properties and FORC distributions) and an unmixing model for isothermal remanent magnetization curves. The paleosol layers in the Mircea Voda sequence experienced significant pedogenic alteration, resulting in high amounts of ultrafine grained SP, grains at SP/SD threshold, stable SD grains and PSD magnetite/maghemite grains. The loess layers in the Mircea Voda sequence are dominated by MD and/or PSD oxidized magnetite probably of aeolian origin. The unmixing model for IRM curves shows the presence of three components with different coercivities. The soft (~21 mT) and medium (~42 mT) coercivity components are produced by pedogenesis during interglacial and interstadial periods. The hard coercivity component (~60 mT) is of aeolian origin, being dominant in loess layers.
机译:介绍了Mircea Voda(罗马尼亚Dobrogea高原)剖面中黄土/古土壤样品的详细岩磁研究。磁粒度仪的气候控制研究使用了几种粒度和浓度相关的代理(磁化率及其频率依赖性,磁滞剩磁,等温剩磁,磁滞特性和FORC分布)和等温剩磁曲线的分解模型。 Mircea Voda序列中的古土壤层经历了明显的成岩作用变化,导致大量的超细颗粒SP,处于SP / SD阈值的颗粒,稳定的SD颗粒和PSD磁铁矿/磁赤铁矿颗粒。 Mircea Voda序列中的黄土层由可能是风成因的MD和/或PSD氧化磁铁矿主导。 IRM曲线的分解模型显示了三种具有不同矫顽力的成分的存在。软(〜21 mT)和中(〜42 mT)矫顽力成分是在间冰期和陆间期通过成岩作用产生的。硬矫顽力成分(〜60 mT)是风成因,在黄土层中占主导地位。

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  • 来源
    《Quaternary International》 |2013年第19期|5-14|共10页
  • 作者单位

    Faculty of Physics, Paleomagnetic Laboratory, University of Bucharest, N. Balcescu 1, 010041 Bucharest, Romania;

    Faculty of Physics, Paleomagnetic Laboratory, University of Bucharest, N. Balcescu 1, 010041 Bucharest, Romania;

    School of Earth Sciences, The Australian National University, Canberra, ACT 0200, Australia;

    Faculty of Physics, Paleomagnetic Laboratory, University of Bucharest, N. Balcescu 1, 010041 Bucharest, Romania;

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