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Uranium series analysis of 2006 augustine volcanics: An investigation into the timescales of magmatic processes.

机译:2006年奥古斯丁火山的铀系列分析:对岩浆过程时间尺度的调查。

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摘要

The purpose of this study is to constrain the mode and tempo of the processes that generated lavas erupted in 2006 eruption from Augustine Volcano, Alaska. There have been 5 eruptions from Augustine over the last century that ejected andesitic to dacitic lava domes and pyroclastic flows. The short recurrence interval of Augustine, in conjunction with the variety of differentiated magma involved in each eruption makes Augustine an ideal location to study magmatic processes such as magma production, magma mixing, magma differentiation, and shallow degassing occurring over the decadal time-scales in explosive subduction-related volcanoes. Toward this end, 2006 Augustine ejecta were analyzed for abundances of short and long-lived U-series nuclides including 238 U, 230Th, 226Ra, and 210Pb as well as the abundances of a complete suite of major and trace elements.;Samples from Augustine have nearly constant Th/U rations, but excesses of (230Th) over (238U) that vary more than the analytical error. Based on documentation for basaltic parental magmas (Larsen et al., 2010) and a lack of evidence for garnet fractionation in differentiated magmas, variations in (230Th/232Th) values for Augustine magmas appear to result from mixing melts and crystals, which have average ages as high as 54 Ka.;Our most mafic sample (an enclave with 53 wt % SiO2) has ( 226Ra/230Th) = ∼1.2. With increasing concentrations of SiO2, the (226Ra/230Th) values decrease to ∼1 at SiO2 ∼ 56 wt%, increase to 1.45 at SiO 2 ∼ 59 wt%, then decrease to ∼1 in samples with >61 wt. % SiO 2. These data suggest that three magmas mingled and mixed during the 2006 eruption: basaltic andesites with Ra excesses generated by mantle melting; a 59 wt% SiO2 magma with 226Ra excesses generated from incongruent melting of young plutonic materials, and 61-62 wt % SiO 2 andesites with relatively long crustal residence times.;Excesses of (210Pb) over (226Ra) were measured in the most mafic and silicic samples at Augustine, whereas intermediate samples had either equilibrium (210Pb/226Ra) or small 210Pb deficits. The excesses in the basaltic andesites were likely generated during degassing within a compositional boundary layer. Excesses in high silica samples were likely produced by localized degassing through porous networks of vesicles.
机译:这项研究的目的是限制从阿拉斯加的奥古斯丁火山爆发的2006年火山喷发中产生熔岩的过程的模式和速度。上个世纪从奥古斯丁爆发了5次喷发,喷出了安山岩到大熔岩穹顶和火山碎屑流。奥古斯丁的短暂复发间隔,再加上每次喷发涉及的分化岩浆种类繁多,使奥古斯丁成为研究岩浆生产,岩浆混合,岩浆分化和年代际时间尺度上发生的浅层脱气等岩浆过程的理想场所。与爆炸物俯冲有关的火山。为此,分析了2006年奥古斯丁喷射器的短寿命U系列核素的丰度,包括238 U,230Th,226Ra和210Pb,以及全套主要和微量元素的丰度。具有几乎恒定的Th / U比率,但是(230Th)超过(238U)的变化幅度大于分析误差。根据有关玄武岩母岩浆的文献(Larsen等,2010),以及缺乏区分岩浆中石榴石分级的证据,奥古斯丁岩浆的(230Th / 232Th)值变化似乎是由熔体和晶体的混合造成的年龄高达54 Ka .;我们最镁铁质的样品(一个含53 wt%SiO2的飞地)的(226Ra / 230Th)=〜1.2。随着SiO2浓度的增加,(226Ra / 230Th)值在SiO2〜56 wt%时降低至〜1,在SiO 2〜59 wt%时升高至1.45,然后在> 61 wt。%的样品中降低至〜1。 %SiO 2。这些数据表明,在2006年喷发过程中,三个岩浆混合并混合在一起:玄武质安山岩,由于地幔融化而产生的Ra过量; 59%的SiO2岩浆,由年轻的深成岩物质不均匀融化产生226Ra过量,地壳停留时间相对较长的61-62 wt%SiO 2安山岩;在最镁铁矿中测得的(210Pb)超过(226Ra)。和奥古斯丁硅质样品,而中间样品具有平衡(210Pb / 226Ra)或较小的210Pb缺陷。玄武质安山岩中的过剩很可能是在组成边界层内的脱气过程中产生的。高二氧化硅样品中的过量可能是由于通过囊泡的多孔网络进行局部脱气而产生的。

著录项

  • 作者

    Thompson, Jennifer Ann.;

  • 作者单位

    The University of Iowa.;

  • 授予单位 The University of Iowa.;
  • 学科 Geochemistry.
  • 学位 M.S.
  • 年度 2011
  • 页码 147 p.
  • 总页数 147
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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