首页> 外文期刊>Bulletin of Volcanology: Journal of the International Association of Volcanology and Chemistry of the Earth s Interior >Total grain size distribution of components of fallout deposits and implications for magma fragmentation mechanisms: examples from Campi Flegrei caldera (Italy)
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Total grain size distribution of components of fallout deposits and implications for magma fragmentation mechanisms: examples from Campi Flegrei caldera (Italy)

机译:岩浆沉积机制的外部沉积物组件的总粒度分布:Campi Flegrei Caldera(意大利)的例子

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摘要

In this paper, we present results of the reconstruction of the total grain size distribution (TGSD) of the material erupted during explosive volcanic eruptions at Campi Flegrei (Italy) considering all components (juvenile, lithic and crystal clasts). To date, the few TGSDs made available have been mostly reconstructed by assuming that the tephra deposits consisted of only one component. This simplification can introduce substantial bias in the interpretation of magma fragmentation mechanisms and significantly affect ash dispersion forecasts, since each tephra component has specific aerodynamic characteristics. By means of field investigations and laboratory analyses on samples collected from deposits of the Agnano-Monte Spina and Astroni eruptions, we reconstructed the TGSDs of juvenile, lithic and crystal components via the Voronoi tessellation method. Our results show how the systematic reconstruction of a TGSD, from the component-specific to the bulk TGSD, can provide important information on magma fragmentation mechanisms and wall-rock erosion processes. Results confirm that the bulk TGSD is the combination of the merging of different component subpopulations, according to their own TGSD, density and relative mass proportions. In addition, the integration of component analysis, TGSD and settling velocity data allowed characterization of the aerodynamic behaviour of each component at variable distances from the vent, which can be related to their own parent grain size distribution. The integration of new data from distal tephra deposits for the considered eruptions has thus allowed a reassessment of the erupted volumes of eruptions considered in this research, which are now 3.17 and 0.63 km(3), for Agnano-Monte Spina and Astroni, respectively.
机译:在本文中,考虑到所有组分(少年,岩石和水晶泥),我们展示了在坎皮山脉(意大利)爆炸性火山喷发期间爆发的材料的总粒度分布(TGSD)的结果。迄今为止,通过假设Tephra存款仅由一个组成部分组成,少数TGSD已经重新构建。这种简化可以在岩浆碎片机制的解释中引入大量偏差,并且显着影响灰分分散预测,因为每个Tephra组分具有特异性的空气动力学特征。通过现场调查和实验室分析来自临床和Astroni爆发的沉积物中收集的样品,我们通过Voronoi曲面细分方法重建了少年,岩石和晶体成分的TGSDS。我们的结果表明,TGSD如何从特定于批量TGSD系统重建,可以提供关于岩浆碎片机制和壁岩侵蚀过程的重要信息。结果证实,散装TGSD根据自己的TGSD,密度和相对质量比例的不同组件亚步骤的合并。另外,组分分析,TGSD和稳定速度数据的集成允许表征来自通风口的可变距离处的每个部件的空气动力学行为,这可以与自己的父粒尺寸分布有关。从远端Tephra沉积物中融合了用于所考虑的爆发的新数据,因此允许重新评估本研究中考虑的爆发的爆发量,现在分别为3.17和0.63公里(3),分别用于Agnano-Monte Spina和Astroni。

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