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Transient Creep and Strain Energy Dissipation: An Experimental Perspective

机译:瞬态蠕变和应变能耗散:实验观点

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Energy dissipation due to intrinsic attenuation occurs at elevated temperatures in rocks as a result of a range of processes. Examples where small-strain, transient deformation occurs are seismic waves, tidal deformation, and at longer timescales post-glacial rebound and far-field post-seismic deformation. Experiments at mantle temperatures and seismic frequencies show that grain boundary sliding is a key process that results in a broad absorption band, as indicated by seismic observations. Models of grain boundary sliding predict a smooth transition from elastic behavior through an anelastic regime toward viscous (Maxwell) behavior, consistent with experimental observations. Other mechanisms that may contribute to dissipation in Earth, at least locally, are dislocations and melt. Extrapolation of the laboratory data shows that first-order observations of planetary behavior and structure can be explained by the effects of temperature and pressure on transient creep properties, but that locally, additional mechanisms are required.
机译:由于固有的衰减,由于一系列过程,能量消耗会在岩石中升高温度时发生。发生小应变,瞬时变形的例子是地震波,潮汐变形,以及在较长的时间尺度上的冰川回弹和远场地震后变形。在地幔温度和地震频率下进行的实验表明,晶界滑动是导致宽吸收带的关键过程,正如地震观测所表明的那样。晶界滑动模型预测了从无弹性状态的弹性行为向粘性(麦克斯韦)行为的平稳过渡,这与实验观察一致。可能至少在局部上有助于地球消散的其他机制是位错和融化。实验室数据的外推表明,行星行为和结构的一阶观测可以通过温度和压力对瞬态蠕变特性的影响来解释,但是局部需要其他机制。

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