首页> 外文期刊>Physics of the Earth and Planetary Interiors: A Journal Devoted to Obsevational and Experimerntal Studies of the Chemistry and Physics of Planetary Interiors and Their Theoretical Interpretation >Electrical resistivity and thermal conductivity of hcp Fe-Ni alloys under high pressure: Implications for thermal convection in the Earth's core
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Electrical resistivity and thermal conductivity of hcp Fe-Ni alloys under high pressure: Implications for thermal convection in the Earth's core

机译:hcp Fe-Ni合金在高压下的电阻率和热导率:对地核中热对流的影响

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We measured the electrical resistivity of Fe-Ni alloys (iron with 5, 10, and 15 wt.% nickel) using four-terminal method in a diamond-anvil cell up to 70 GPa at 300 K. The results demonstrate that measured resistivity increases linearly with increasing nickel impurity concentration, as predicted by the Matthiessen's rule. The impurity resistivity is predominant at ambient temperature; the incorporation of 5 wt.% nickel into iron doubles the electrical resistivity at 60 GPa. Such impurity effect becomes minor at high temperature of the Earth's core because of the resistivity "saturation". We also calculated that >0.9 TW heat flow is necessary at the top of the inner core for thermal convection in the inner core. It requires the CMB heat flow of similar to 30 TW, which is much higher than recent estimates of 5-15 TW. This means that purely thermal convection does not occur in the inner core. (C) 2015 Elsevier B.V. All rights reserved.
机译:我们使用四端子法在300 K高达70 GPa的金刚石-砧式电池中使用四端子法测量了Fe-Ni合金(含5、10和15 wt%的镍的铁)的电阻率。结果表明,测得的电阻率会增加如Matthiessen法则所预测,镍杂质浓度呈线性增加。杂质电阻在环境温度下占主导地位;在铁中加入5 wt。%的镍会使60 GPa的电阻率增加一倍。由于电阻率“饱和”,这种杂质效应在地球核心的高温下变得很小。我们还计算出,在内芯顶部需要大于0.9 TW的热流,以实现内芯的热对流。它要求CMB的热流量接近30 TW,远高于最近估计的5-15 TW。这意味着在内核中不会发生纯粹的热对流。 (C)2015 Elsevier B.V.保留所有权利。

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