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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 >Implications of grain size evolution on the seismic structure of the oceanic upper mantle
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Implications of grain size evolution on the seismic structure of the oceanic upper mantle

机译:粒度演化对海洋上地幔地震结构的影响

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摘要

We construct a 1-D steady state channel flow model for grain size evolution in the oceanic upper mantle using a composite diffusion-dislocation creep theology. Grain size evolution is calculated assuming that grain size is controlled by a competition between dynamic recrystallization and grain growth. Applying this grain size evolution model to the oceanic upper mantle we calculate grain size as a function of depth, seafloor age, and mantle water content. The resulting grain size structure is used to predict shear-wave velocity (Vs) and seismic quality factor (Q). For a plate age of 60 Myr and an olivine water content of 1000 H/10(6)Si, we find that grain size reaches a minimum of similar to 15 mm at similar to 150 km depth and then increases to similar to 20-30 mm at a depth of 400 km. This grain size structure produces a good fit to the low seismic shear-wave velocity zone (LVZ) in oceanic upper mantle observed by surface wave studies assuming that the influence of hydrogen on anelastic behavior is similar to that observed for steady state creep. Further it predicts a viscosity of similar to 10(19) Pa.s at 150 km depth and dislocation creep to be the dominant deformation mechanism throughout the oceanic upper mantle, consistent with geophysical observations. We predict larger grain sizes than proposed in recent studies, in which the LVZ was explained by a dry mantle and a minimum grain size of 1 mm. However, we show that for a 1 mm grain size, diffusion creep is the dominant deformation mechanism above 100200 km depth, inconsistent with abundant observations of seismic anisotropy from surface wave studies. We therefore conclude that a combination of grain size evolution and a hydrated upper mantle is the most likely explanation for both the isotropic and anisotropic seismic structure of the oceanic upper mantle. Our results also suggest that melt extraction from the mantle will be significantly more efficient than predicted in previous modeling studies that assumed grain sizes of similar to 1 mm.
机译:我们使用复合扩散-位错蠕变神学为海洋上地幔中的晶粒尺寸演化构建了一维稳态通道流模型。假设晶粒大小受动态再结晶和晶粒长大之间的竞争控制,则计算晶粒大小的演变。将这种粒度演化模型应用于海洋上地幔,我们可以计算出深度,海底年龄和地幔含水量的函数。所得的晶粒尺寸结构用于预测剪切波速度(Vs)和地震品质因数(Q)。对于板龄为60 Myr的橄榄石水含量为1000 H / 10(6)Si,我们发现,在接近150 km的深度处,晶粒尺寸最小达到类似于15 mm的最小值,然后增加至类似于20-30毫米,深度为400公里。假设氢对非弹性行为的影响与稳态蠕变相似,那么这种晶粒尺寸结构可以很好地拟合海洋上地幔的低地震剪切波速度带(LVZ)。此外,它还预测了在150 km深度处粘度类似于10(19)Pa.s和位错蠕变是整个海洋上地幔的主要变形机制,这与地球物理观测一致。我们预测比最近的研究中提出的建议更大的晶粒尺寸,在LVZ中,LVZ是由干燥的地幔解释的,最小晶粒尺寸为1 mm。但是,我们表明,对于1mm的晶粒,扩散蠕变是100200 km深度以上的主要变形机制,这与表面波研究对地震各向异性的大量观测结果不一致。因此,我们得出的结论是,粒度演化与水合上地幔的结合是海洋上地幔各向同性和各向异性地震结构的最可能解释。我们的结果还表明,从地幔中提取熔体将比以前的模拟研究(假定颗粒大小近似于1毫米)中预测的效率高得多。

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