バン! バン! サントリーニの火山で月間規模の噴火が起きました.
Victoria M Martin1, Daniel J Morgan, Dougal A Jerram
1University of Durham, Department of Earth Sciences, South Road, Durham DH1 3LE, UK.
まとめ
研究者は,マグマの侵入と噴火の間の時間を決定するために,ギリシャのサントリーニの火山物質を研究しました. オリヴィン結晶解析を用いて,この臨界時間遅延が3~10週間と判明した.
科学分野:
- 地質学 地質学 地質学
- 火山学 火山学とは
- 地質化学 地質化学
背景:
- マグマの侵入と火山噴火の間の時間は,火山の活動を予測し,危険を軽減するために重要です.
- この時間スケールを理解することは,火山噴火の引き金と結果を評価するのに役立ちます.
研究 の 目的:
- ギリシャのサントリーニにあるネア・カメニ火山の中心での侵入から噴火までの時間の遅れを決定するために.
- 火山の過程の研究のために,以前に噴火した材料に分析技術を適用する.
主な方法:
- ネアカメニの1925~28年の噴火からのオリヴィン結晶におけるFe-Mg拡散の分析.
- 地化学技術を用いて火山材料の熱史を再構築する.
主要な成果:
- 侵入から噴火までの時間の遅れは3〜10週間の期間に制限されました.
- この研究では,歴史的な噴火材料を使用して,短期的な火山のプロセスを成功裏に校正しました.
結論:
- オリビンのFe-Mg拡散は,マグマの侵入から噴火までの時間スケールを決定するための信頼できる方法を提供します.
- この技術は他の火山の中心にも適用され,火山のプロセスを研究する能力を高めます.
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