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首页> 外文期刊>Contributions to Mineralogy and Petrology >Magnesian andesite and dacite lavas from Mt. Shasta, northern California: products of fractional crystallization of H_2O-rich mantle melts
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Magnesian andesite and dacite lavas from Mt. Shasta, northern California: products of fractional crystallization of H_2O-rich mantle melts

机译:芒特山的镁质安山岩和达克特熔岩。加利福尼亚州北部的沙斯塔:富H_2O地幔熔体的分步结晶产物

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Mt. Shasta andesite and dacite lavas contain high MgO (3.5-5 wt. percent), very low FeO*/MgO (1-1.5) and 60-66 wt. percent SiO_2. The range of major and trace element compositions of the Shasta lavas can be explained through fractional crystallization (approx 50-60 wt. percent) with subsequent magma mixing of a parent magma that had the major element composition of an H_2O-rich primitive magnesian andesite (PMA). Isotopic and trace element characteristics of the Mt. Shasta stratocone lavas are highly variable and span the same range of compositions that is found in the parental basaltic andesite and PMA lavas. This variability is inherited from compositional variations in the input contributed from melting of mantle wedge peridotite that was fluxed by a slab-derived, fluid-rich component. Evidence preserved in phenocryst assemblages indicates mixing of magmas that experienced variable amounts of fractional crystallization over a range of crustal depths from approx 25 to approx 4 km beneath Mt. Shasta. Major and trace element evidence is also consistent with magma mixing. Pre-eruptive crystallization extended from shallow crustal levels under degassed conditions (approx 4 wt. percent H_2O) to lower crustal depths with magmatic H_2O contents of approx 10-15 wt. percent. Oxygen fugacity varied over 2 log units from one above to one below the Nickel-Nickel Oxide buffer. The input of buoyant H_2O-rich magmas containing 10-15 wt. percent H_2O may have triggered magma mixing and facilitated eruption. Alternatively, vesiculation of oversaturated H_2O-rich melts could also play an important role in mixing and eruption.
机译:公吨。 Shasta安山岩和辉绿岩熔岩包含高含量的MgO(3.5-5 wt%),非常低的FeO * / MgO(1-1.5)和60-66 wt%。 SiO_2百分比。 Shasta熔岩的主要和微量元素组成的范围可以通过分步结晶(约50-60 wt。%)以及随后的母岩浆的岩浆混合来解释,该母岩浆具有富含H_2O的原始镁质安山岩的主要元素组成( PMA)。山的同位素和微量元素特征。 Shasta Stratocone熔岩变化很大,其组成范围与亲本玄武质安山岩和PMA熔岩相同。这种变异性是从地幔楔形橄榄岩熔融引起的输入成分变化中继承的,而地幔楔形橄榄岩的熔融是由板坯衍生的富流体成分助熔的。隐晶组合中保存的证据表明,在Mt下方约25至约4 km的地壳深度范围内,经历了不同程度的分步结晶的岩浆混合。沙斯塔。主要和微量元素证据也与岩浆混合一致。喷发前的结晶作用从脱气条件下的浅地壳水平(大约4 wt。%H_2O)扩展到较低的地壳深度,岩浆H_2O含量大约为10-15 wt%。百分。氧气逸度从2个对数单位变化,从上一下到下一氧化镍缓冲液。含10-15 wt%的浮力丰富的H_2O岩浆的输入。 H_2O百分比可能已触发岩浆混合并促进了喷发。另外,过饱和的富H_2O熔体的囊泡化也可能在混合和喷发中起重要作用。

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