火山学. 火山学について. トバ・カルデラの下にある大きなマグマティック・スリープ・コンプレックス
K Jaxybulatov1, N M Shapiro2, I Koulakov3
1Trofimuk Institute of Petroleum Geology and Geophysics, Siberian Branch of Russian Academy of Sciences, Prospekt Koptyuga, 3, Novosibirsk, 630090 Russia. Novosibirsk State University, 2, Pirogova Street, Novosibirsk 630090, Russia. Institut de Physique du Globe de Paris, Sorbonne Paris Cité, CNRS (UMR 7154), 1 rue Jussieu, 75238 Paris, Cedex 5, France.
まとめ
超火山を養うような大きな火山貯水池は,広大なシール複合体として形成されることがあります. この発見は,主要な火山噴火につながるマグマ体の漸進的な進化を支持しています.
科学分野:
- 地質物理学 地質物理学とは地質物理学です.
- 火山学 火山学とは
- 地震学 地震学とは
背景:
- 大規模なマグマ貯水池の形成を理解することは,将来の火山噴火リスクを評価するために不可欠です.
- 超火山は地球規模で大きな脅威となり,マグマ系の研究が求められている.
研究 の 目的:
- 地震アニソトロピーを用いて主要な火山貯水池の大きさと成熟度を推定する.
- トバ・カルデラのマグマシステムの構造を調査するために.
主な方法:
- 周囲の騒音による地震トモグラフィーは,トバ・カルデラの下部で使用された.
- 放射性地震アニソトロピーは,地下構造を推論するために分析されました.
主要な成果:
- 地震アニソトロピーは,深さ7km未満の微細層層構造を示しています.
- この層は,地殻内の多数の部分的に溶けたスリープとして解釈されます.
- トバマグマ貯水池は,大きなスリープ複合体であるようです.
結論:
- 超火山のマグマ貯水池は,広範囲のシール複合体として発展することができます.
- これは,大規模な噴火につながる長期的,漸進的なマグマ体の進化の理論を支持します.
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