岩石气体的组成揭示了子驱动的斯特伦波利亚爆炸活动的源头深度
Mike Burton1, Patrick Allard, Filippo Muré
1Istituto Nazionale di Geofisica e Vulcanologia, Catania, Italy. burton@ct.ingv.it
概括
推动斯特罗姆波尔喷发的气体在火山地接口的深处形成,深度约为3公里. 这种深层起源解释了在斯特伦博利火山观察到的形形成和浅层爆炸地震之间的脱节.
科学领域:
- 火山学 火山学是一门学科.
- 地质物理学 地质物理学
- 地质化学 地质化学
背景情况:
- 斯特伦波尔喷发的特点是气爆炸,但它们的形成深度和机制尚不清楚.
- 爆炸的地震性通常很浅,造成了关于深层岩过程的知识差距.
- 了解形成对于解释火山动荡和火山爆发动态至关重要.
研究的目的:
- 为了确定对斯特伦波尔喷发负责的气体的起源深度.
- 研究控制气凝聚和上升的过程.
- 为了阐明深层的起源和浅层地震信号之间的关系.
主要方法:
- 在Stromboli火山的静止脱气和爆炸阶段进行光谱测量.
- 分析气体组成和气泡动态.
- 光谱数据与地震记录的相关性.
主要成果:
- 气起源于火山-地接口 (约. 3公里) 的距离.
- 结构不连续性和差异性泡上升促进了深处的菌凝聚.
- 在深层形成和浅层爆炸地震之间存在脱 (约. 250 公里).
结论:
- 斯特罗姆波尔活动中的气起源发生在相当深处,而不仅仅是浅层.
- 火山管道系统的几何决定了观察到的地震信号和喷发风格.
- 这种深层起源模型可能适用于全球其他斯特伦波利火山.
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