Tongzhang Qu , Ian Jackson , Ulrich H. Faul , Emmanuel C. David
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However, these observations may have been complicated by the austenite to ferrite plus cementite phase transition in the jacket material, compliance associated with interfacial Ni<sub>70</sub>Fe<sub>30</sub> foils, and modeling of the mechanical properties of polycrystalline alumina as control specimen. To investigate the influence of these complications within the experimental setup and provide forced-oscillation data of better quality especially at moderate temperatures, we have conducted further forced-oscillation tests for which we removed the interfacial foils, employed single-crystal sapphire as reference sample, and used alternative jacket materials (stainless steel or copper) which experience no phase transition during the staged cooling. The newly acquired forced-oscillation data, although broadly consistent with the previous results, differ significantly especially in temperature sensitivity, and allow refinement of an appropriate Burgers creep-function model. 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引用次数: 0
摘要
微观力学模型表明,多晶橄榄石中弹性松弛的起始点应该是一个由弹性容纳的晶界滑动引起的轻度耗散峰,这对解释上地幔中的地震波衰减和频散至关重要。在以前对置于软钢夹套中的细粒白云石进行的强制振荡实验中,这种行为被初步用来解释短周期剪切模量不足和在 900-700 °C时难以解析的耗散高原。然而,夹套材料中从奥氏体到铁素体加雪明体的相变、与界面镍铁箔相关的顺应性以及作为对照试样的多晶氧化铝的力学性能建模,都可能使这些观察结果变得复杂。为了研究实验装置中这些复杂因素的影响,并提供更高质量的强制振荡数据(尤其是在中等温度下),我们进行了进一步的强制振荡测试,去除了界面箔,使用单晶蓝宝石作为参考样品,并使用了在分段冷却过程中不会发生相变的其他夹套材料(不锈钢或铜)。新获得的强迫振荡数据虽然与之前的结果基本一致,但尤其在温度敏感性方面存在显著差异,因此可以完善适当的布尔格斯蠕变函数模型。在温度约为 950-1050 °C、地震周期为 1-1000 s 的干燥、无熔体和细粒度白云石中,在弹性松弛开始时,单调松弛背景上叠加了一个温和的耗散峰。同时涉及耗散和相关分散的粘弹性行为的高活化能(> 600 kJ/mol)表明,晶界扩散可能受到晶界内界面反应的限制。
The onset of anelastic behavior in fine-grained synthetic dunite
Micromechanical models suggest that the onset of anelastic relaxation in polycrystalline olivine, critical to interpretation of the seismic wave attenuation and dispersion in the upper mantle, should be a mild dissipation peak caused by elastically accommodated grain-boundary sliding. Such behavior has been tentatively invoked to explain both a short-period shear modulus deficit and a dissipation plateau poorly resolved at 900–700 °C in previous forced-oscillation experiments on fine-grained dunite tested within mild-steel jackets. However, these observations may have been complicated by the austenite to ferrite plus cementite phase transition in the jacket material, compliance associated with interfacial Ni70Fe30 foils, and modeling of the mechanical properties of polycrystalline alumina as control specimen. To investigate the influence of these complications within the experimental setup and provide forced-oscillation data of better quality especially at moderate temperatures, we have conducted further forced-oscillation tests for which we removed the interfacial foils, employed single-crystal sapphire as reference sample, and used alternative jacket materials (stainless steel or copper) which experience no phase transition during the staged cooling. The newly acquired forced-oscillation data, although broadly consistent with the previous results, differ significantly especially in temperature sensitivity, and allow refinement of an appropriate Burgers creep-function model. A mild dissipation peak superimposed on monotonic dissipation background during the onset of anelastic relaxation in dry, melt-free and fine-grained dunite has now been consistently observed at temperatures of ∼950–1050 °C and seismic periods of 1–1000 s. Such a dissipation peak with relaxation strength 0.02 ± 0.01 is attributed to elastically accommodated grain-boundary sliding. The high activation energy (> 600 kJ/mol) of viscoelastic behavior involving both dissipation and related dispersion suggests that grain-boundary diffusion may be limited by interfacial reaction within grain boundaries. The reduced relaxation strength makes it difficult to attribute the oceanic lithosphere-asthenosphere boundary to water-mediated elastically accommodated grain-boundary sliding.
期刊介绍:
Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. It is the only journal to be entirely devoted to the physical and chemical processes of planetary interiors.
Original research papers, review articles, short communications and book reviews are all published on a regular basis; and from time to time special issues of the journal are devoted to the publication of the proceedings of symposia and congresses which the editors feel will be of particular interest to the reader.