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Constraining magma storage conditions using phase equilibria models at a restless volcano in the Main Ethiopian Rift

机译:使用相平衡模型在埃塞俄比亚主裂谷的不​​安火山中限制岩浆储存条件

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摘要

The Main Ethiopian Rift hosts a number of peralkaline volcanic centres, with many showing signs of recent unrest. Due, in part, to the low number of historical eruptions recorded in the region, volcanism in the Main Ethiopian Rift remains understudied relative to other volcanic settings and conditions of magma storage remain almost entirely unknown. Aluto is one of these restless caldera systems and identifying magma storage conditions is vital for evaluating the risks posed by recent periods of unrest. In this study, we ran ~ 150 fractional crystallisation models, using the Rhyolite-MELTS thermodynamic software, within the range = 50–300 MPa, starting HO = 0.5–3 wt% and O = QFM-2 − QFM + 1. This represents a realistic range of potential magma storage conditions at Aluto. We assessed the fractionation trends produced using two different starting compositions, which represent different estimates of the parental melt feeding the system. The predicted liquid lines of descent produced by these models are compared with Aluto whole-rock data from the literature, and are presented along with new observations of the natural phase assemblage and erupted mineral compositions to provide information on the magma storage conditions.Using a new, quantitative statistical approach to compare empirical data and thermodynamic model-outputs, we find that the compositions of evolved peralkaline rhyolites from Aluto are best reproduced by isobaric fractional crystallisation from a rift-related basaltic composition, without the need for significant crustal assimilation. Around 90% protracted fractional crystallisation is required to produce these compositions. This indicates that the magmatic system is likely to exist as a highly crystalline mush. The best agreement between models and natural samples is at low pressures (150 MPa), low initial HO concentrations (0.5 wt%) and relatively high oxygen fugacity (QFM). The depth of magma storage derived from these results (~ 5.6 ± 1 km) agrees well with the source depths modelled from measured ground deformation at Aluto in 2008. Data from other peralkaline volcanic centres in the Main Ethiopian Rift, such as Boset and Gedemsa, and at other locations globally (e.g. Pantelleria, Italy) suggest that these storage conditions are a common feature of many peralkaline volcanic centres. Our data is consistent with the formation of a Daly Gap at Aluto due to compositional stratification of the magma reservoir beneath the caldera, and the non-linear relationship between temperature and SiO concentration during magmatic differentiation.
机译:埃塞俄比亚主要裂谷拥有许多碱性的火山中心,其中许多都显示出近期动荡的迹象。部分原因是由于该地区记录的历史喷发数量少,相对于其他火山环境,埃塞俄比亚主要裂谷的火山活动仍处于研究不足状态,岩浆储存条件几乎完全未知。冥王星是这些不安定的破火山口系统之一,识别岩浆储存条件对于评估近期动乱带来的风险至关重要。在这项研究中,我们使用Rhyolite-MELTS热力学软件运行了〜150个分步结晶模型,范围为= 50–300 MPa,起始HO = 0.5–3 wt%,O = QFM-2 − QFM +1。这表示Aluto的潜在岩浆储存条件的实际范围。我们评估了使用两种不同的起始组分产生的分馏趋势,这代表了对母体熔体进料系统的不同估计。将这些模型产生的预测下降液体线与文献中的Aluto全岩数据进行比较,并与自然相组合和喷出的矿物成分的新观察结果一起提供,以提供有关岩浆储存条件的信息。定量统计方法来比较经验数据和热力学模型的输出结果,我们发现从裂谷相关的玄武岩成分中进行等压重结晶可以最好地重现Aluto演化出的碱性碱性流纹岩的成分,而无需进行大量的地壳同化作用。生产这些组合物需要约90%的延长的分步结晶。这表明岩浆系统很可能以高度结晶的糊状物形式存在。模型与自然样品之间的最佳协议是在低压(150 MPa),低初始HO浓度(0.5 wt%)和相对较高的氧逸度(QFM)下。从这些结果得出的岩浆储存深度(约5.6±1 km)与2008年在Aluto测得的地面变形所模拟的震源深度非常吻合。埃塞俄比亚大裂谷其他碱性碱性火山中心的数据,例如Boset和Gedemsa,在全球其他地方(例如意大利潘泰莱里亚),则表明这些储存条件是许多高碱性火山岩中心的共同特征。我们的数据与火山口下方岩浆储层的成分分层,以及在岩浆分化过程中温度和SiO浓度之间的非线性关系有关,在铝层上形成了Daly Gap。

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