日本地球惑星科学連合2025年大会

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[J] ポスター発表

セッション記号 M (領域外・複数領域) » M-GI 地球科学一般・情報地球科学

[M-GI29] データ駆動地球惑星科学

2025年5月26日(月) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:上木 賢太(国立研究開発法人海洋研究開発機構)、伊藤 伸一(東京大学)、板野 敬太(秋田大学)、宇野 正起(東京大学大学院理学系研究科地球惑星科学専攻)

17:15 〜 19:15

[MGI29-P05] 黒潮流軸の類似検索を用いたデータ駆動型軽石漂流推移予測:伊豆諸島明神礁への適用

*桑谷 立1、日野 英逸2、西川 遥1、赤穂 昭太郎3,2 (1.海洋研究開発機構、2.統計数理研究所、3.産業技術総合研究所)

キーワード:漂流軽石、データ駆動、海流、自然災害

Pumice raft drift has recently been recognized as a new disaster risk, and predicting its distribution patterns is crucial for ensuring safe maritime navigation and implementing timely coastal disaster mitigation measures. While drift simulations based on ocean current patterns have proven effective, conducting such physical simulations immediately after an eruption requires significant preparation time, human resources, and computational costs. Since eruptions are unpredictable and often small in scale, establishing a real-time prediction method that can serve as an alternative to physical simulations is an urgent issue. This study aims to develop a methodology for real-time drift pattern prediction by searching for similar patterns in daily-reported Kuroshio Current axis data, eliminating the need for physical simulations. We conducted validation tests using existing data under the assumption of a pumice eruption at Myojinsho, the Izu Islands, where the Kuroshio Current axis frequently passes nearby. The results demonstrated that the use of Dynamic Time Warping (DTW), a distance metric that measures similarity based on the overall alignment of directed paths, enables relatively accurate predictions of drift patterns over a 10-day period.