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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 >Tracing the differences between Vulcanian and Strombolian explosions using infrasonic and thermal radiation energy
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Tracing the differences between Vulcanian and Strombolian explosions using infrasonic and thermal radiation energy

机译:利用次声和热辐射能追踪伏尔加尼亚爆炸和斯特伦伯利亚爆炸之间的差异

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摘要

Eruptive plume dynamics is a direct expression of explosive style, where duration and altitude of eruptive clouds and dispersion of erupted products is proportional to the degree of fragmentation. We present an analysis of infrasonic and thermal records for explosions at Villarrica (Chile), Stromboli (Italy), Santiaguito and Fuego (Guatemala) volcanoes. Across these four systems magma composition spans from basaltic to dacitic and explosive activity is typically described as ranging from Strombolian to Vulcanian. We use this analysis to provide a quantitative, geophysically-based description of, and discrimination between, the different explosive styles that characterize the four volcanoes. While infrasound is directly related to the emission of over-pressurized gas, and thus solely reflects the plume emission, both plume emission and ascent are detected thermally. Thus, the two data sets together provide a complete description of the plume dynamics. In particular, while infrasound solely reflects the gas-thrust phase driving plume emission, thermal radiation energy is also affected by buoyancy during plume ascent. Thermal radiation energy estimated for explosions at Stromboli and Villarrica (10~4-10~7?J) is lower than that for events at Santiaguito and Fuego (10~8-10~9?J), but infrasonic energies overlap. This suggests a greater contribution of buoyancy for eruptive clouds at Santiaguito and Fuego when compared with Stromboli and Villarrica. We further investigated the plume dynamics by comparing infrasonic energy, which reflects gas-thrust (E_(GT)), with the difference between thermal radiation and infrasonic energies, which mostly reflects buoyancy (E_B). Our data distribution reveals two separate clusters. Explosions at Stromboli and Villarrica share low values of buoyancy, pointing to a gas-thrust dominated emission, efficient coupling of the infrasonic source to the atmosphere, and a Strombolian-type source process to generate a plume rich in coarse fragments. In contrast, explosions at Santiaguito and Fuego share large buoyancy (E_B), and are consistent with Vulcanian-type events in which a large part of infrasonic energy is spent in magma fragmentation leading to ascent of buoyant, ash-rich plumes. We demonstrate that the comparison between thermal radiation and infrasonic energies of explosions allows a quantitative discrimination between, and characterization of, Strombolian- and Vulcanian-type explosions, which leads us to suggest that such an approach may be used as an index to further (and quantitatively) discriminate between eruptive styles.
机译:爆发羽流动力学是爆发式的直接表达,其中爆发云的持续时间和高度以及爆发产物的散布与破碎程度成正比。我们提供了对Villarrica(智利),Stromboli(意大利),Santiaguito和Fuego(危地马拉)火山爆炸的次声和热记录的分析。在这四个系统中,岩浆成分范围从玄武岩到达格岩,爆炸性活动通常被描述为从斯特伦波斯时期到伏尔加山脉。我们使用这种分析来提供基于地球物理的定量描述,并区分这四种火山的不同爆炸样式。次声与过压气体的排放直接相关,因此仅反映了羽流的排放,而羽流的排放和上升都是热检测的。因此,这两个数据集一起提供了羽流动力学的完整描述。尤其是,次声仅反映了推动推流羽流的气相推力阶段,而在推升羽流过程中,热辐射能也受到浮力的影响。 Stromboli和Villarrica(10〜4-10〜7?J)爆炸的热辐射能量估计低于Santiaguito和Fuego(10〜8-10〜9?J)的事件的热辐射能量,但次声能量重叠。这表明,与斯特龙博利和维拉里卡相比,浮力对Santiaguito和Fuego的爆发云的贡献更大。我们通过比较反映气体推力的次声能(E_(GT)),热辐射和次声能之间的差异(主要反映浮力)来进一步研究羽流动力学。我们的数据分布揭示了两个单独的集群。 Stromboli和Villarrica的爆炸物的浮力值很低,表明以气体推力为主的排放,次声源与大气的有效耦合以及Strombolian型源过程产生了富含粗碎屑的羽流。相比之下,Santiaguito和Fuego的爆炸具有较大的浮力(E_B),并且与Vulcanian类型的事件一致,在该事件中,大部分次声能被消耗在岩浆碎裂中,导致浮力高,富含灰分的烟羽上升。我们证明了爆炸的热辐射与次声能之间的比较允许对Strombolian型和Vulcanian型爆炸进行定量区分和表征,这使我们建议这种方法可以用作进一步(和定量地)区分喷发样式。

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