Emplacement dynamics of a crystal-rich, highly viscous trachytic flow of the Sancy stratovolcano, France

GSA Bulletin Pub Date : 2022-12-06 DOI:10.1130/b36415.1
Jean-Marie Prival, A. Harris, E. Zanella, Claudio Robustelli Test, L. Gurioli, O. Chevrel, Jonas Biren
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引用次数: 2

Abstract

Emplacement dynamics of highly viscous, silicic lava flows remain poorly constrained due to a lack of consideration of crystal-rich cases. Emplacement models mostly apply to glassy or microlitic, vesiculated rhyolitic flows. However, crystalline, vesicle-free silicic lava can flow differently. We studied the Grande Cascade unit, which is a vesicle-free, phenocryst-rich, trachytic flow in the Monts Dore massif, France. Field work was carried out to define internal structures, and oriented samples were collected for chemical, petrological, and anisotropy of magnetic susceptibility analyses, allowing us to estimate emplacement temperature and viscosity. These data allow us to define a new silicic lava flow subtype that is low in temperature (800−900 °C), high in silica content (up to 66.8 wt%), high in viscosity (109−1011 Pa s), rich in phenocrysts (∼35%), and lacks vesicles. Brittle deformation of the lava occurs upon extrusion, generating a cataclasite basal layer and thin (3-m-thick) shear zone that accommodates all of the stress, allowing most of the flow’s volume to slide over its base as a 40-m-thick plug in which there is no deformation. Blocks are rare, of a single size (10 ± 1 cm), and result from localized break-up of the basal shear zone. Emplacement dynamics are different from those of glassy, pumiceous lava flows. They are closer to glacier dynamics, where most of the volume slides over a thin basal shear zone and till is generated there by abrasion and milling of the underlying layer. For the Grande Cascade lava flow, abrasion means that the flow lacks its classical blocky crust and instead the flow base is marked by a layer rich in fine-grained material. The structures and emplacement dynamics of this crystal-rich flow are consistent with ideal, gravity-driven shear flow. We thus argue for a global reassessment of silicic-rich lava emplacement based on crystal content and using a multidisciplinary approach focused on well-exposed examples in the rock record.
法国Sancy层状火山富含晶体的高粘性粗流的就位动力学
由于缺乏对富含晶体的情况的考虑,高粘性、硅质熔岩流的就位动力学仍然很不受约束。就位模型主要适用于玻璃状或微晶状、囊状流纹岩流动。然而,结晶的、无囊泡的硅熔岩可以以不同的方式流动。我们研究了大瀑布单元,这是一个无囊泡,富含斑晶,在法国多雷山地块的浅裂流。现场工作确定了内部结构,并收集定向样品进行化学、岩石学和磁化率各向异性分析,使我们能够估计就位温度和粘度。这些数据使我们能够定义一种新的硅质熔岩流亚型,其温度低(800 - 900°C),硅含量高(高达66.8 wt%),粘度高(109 - 1011 Pa s),富含斑晶(~ 35%),缺乏囊泡。岩浆在挤压时发生脆性变形,形成碎裂岩基底层和薄的(3米厚)剪切带,可以容纳所有的应力,允许大部分流量在其底部滑动,形成40米厚的堵塞,其中没有变形。块体罕见,大小单一(10±1 cm),是基底剪切带局部破碎的结果。就位动力学不同于玻璃状、浮石状的熔岩流。它们更接近冰川动力学,在那里,大部分体积在一个薄的基底剪切带上滑动,在那里,土壤是由下层的磨损和研磨产生的。对于大喀斯喀特熔岩流来说,磨损意味着该流缺少其典型的块状地壳,而流底则以一层富含细颗粒物质的地层为标志。这种富晶流的结构和就位动力学符合理想的重力驱动剪切流。因此,我们主张以晶体含量为基础,采用多学科方法,重点研究岩石记录中暴露良好的例子,对富硅熔岩就位进行全球重新评估。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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