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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 >Grain growth systematics for forsterite +/- enstatite aggregates: Effect of lithology on grain size in the upper mantle
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Grain growth systematics for forsterite +/- enstatite aggregates: Effect of lithology on grain size in the upper mantle

机译:镁橄榄石+/-顽辉石聚集体的晶粒长大系统:岩性对上地幔晶粒尺寸的影响

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Grain growth kinetics of forsterite (Fo) and enstatite (En) in fine grain aggregates of Fo En are examined as a function of volume fraction of En (f(En) = 0.00 to 0.42). Growth rates fit d(n)proportional to k . t (d: mean grain diameter; n: grain growth exponent: k: growth constant; t: time), where n similar to 5 for both forsterite and enstatite grains in the enstatite-bearing samples. A negative correlation between k(Fo) and f(En) can be expressed as k(Fo)approximate to 0.06 exp [30 f(En) (f(En) - 1.1)], whereas k(En) takes almost constant values for different f(En). In addition, the ratio of d(Fo)/d(En) is almost constant during grain growth, and its value becomes smaller with increasing An, such that d(Fo)/d(En)approximate to 0.74/f(En)(0.59). Our obtained grain growth parameters and the microstructural characteristics in experimental and natural samples all indicate that the rate-controlling process for grain growth in both experiments and in nature is grain boundary diffusion of Si through grain boundaries of olivine. Thus, we are able to propose a semi-empirical relationship of d(Av)e / d(dun) approximate to {exp[30f(px)-1.1)]}(1/5).(1 + 1.35f(px)(1.59)-f(px)) (d(Ave), : average grain size in the rock; d(dun): average grain size in dunite:f(px):fraction of pyroxenes), which can predict how lithology affects grain size in the upper mantle. Grain size in lherzolite (pyroxenes content of 40%) can be similar to 4 times smaller than that in dunite (pyroxenes content of 5%). Such grain size reduction through change in lithology can significantly affect viscosity of mantle deformation via grain-size sensitive creep.
机译:研究了Fo En细粒聚集体中镁橄榄石(Fo)和顽辉石(En)的晶粒生长动力学,其与En体积分数的关系(f(En)= 0.00至0.42)。增长率适合d(n)与k成正比。 t(d:平均晶粒直径; n:晶粒生长指数:k:生长常数; t:时间),其中在含顽石的样品中镁橄榄石和顽辉石晶粒的n均类似于5。 k(Fo)和f(En)之间的负相关可以表示为k(Fo)约等于0.06 exp [30 f(En)(f(En)-1.1)],而k(En)几乎取恒定值对于不同的f(En)。另外,d(Fo)/ d(En)的比率在晶粒生长期间几乎恒定,并且其值随着An的增加而变小,使得d(Fo)/ d(En)近似为0.74 / f(En)。 (0.59)。我们获得的晶粒生长参数以及在实验和自然样品中的微观结构特征均表明,在实验和自然界中,晶粒生长的速率控制过程都是Si通过橄榄石晶界扩散的晶界。因此,我们能够提出近似于{exp [30f(px)-1.1)]}(1/5)的d(Av)e / d(dun)的半经验关系。(1 + 1.35f(px) )(1.59)-f(px))(d(Ave),:岩石中的平均晶粒度; d(dun):榴辉岩中的平均晶粒度:f(px):辉石的分数),可以预测岩性影响上地幔的粒度。锂铁矿(辉石含量为40%)中的晶粒尺寸可以类似于榴辉岩(辉石含量为5%)中晶粒尺寸的4倍。由于岩性变化而导致的这种晶粒尺寸减小会显着影响通过晶粒尺寸敏感性蠕变引起的地幔变形粘度。

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