日本地球惑星科学連合2018年大会

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セッション記号 H (地球人間圏科学) » H-DS 防災地球科学

[H-DS07] 地すべりおよび関連現象

2018年5月22日(火) 10:45 〜 12:15 201B (幕張メッセ国際会議場 2F)

コンビーナ:千木良 雅弘(京都大学防災研究所)、王 功輝(京都大学防災研究所)、今泉 文寿(静岡大学農学部)、座長:今泉 文寿

11:45 〜 12:00

[HDS07-11] Influence of grain-size distribution on formation of debris-flow fan

*經隆 悠1堀田 紀文2酒井 佑一2西口 幸希3日名 純也3 (1.筑波大学生命環境科学研究科、2.東京大学大学院農学生命科学研究科、3.株式会社建設技術研究所)

キーワード:土石流、土石流扇状地、水路実験、PIV、SfM

Accurate prediction of debris-flow fan formation is critical to sediment disaster mitigation because most damage from debris flow occurs in the inundation area. Although actual debris flows include a diversity of grain sizes, assessment is generally based on numerical simulation results for monogranular debris flows. This study conducted flume tests of debris flows using 0.08 m3 of sediment particles that were either monogranular (2.65 mm) or a mixture of seven diameters (0.7 to 6 mm; average size of 2.65 mm) and compared formation processes of debris-flow fans to examine the influence of grain-size distribution. Channels (15°, 10 cm wide) with a deposition area (12° to 6°) were used for the experiments. We captured the development of the debris-flow fans using photographs and videos made by digital cameras and used the techniques of Structure from Motion (SfM) and Particle Image Velocimetry (PIV) to monitor debris-flow fan formation and flow regimes. As a result, monogranular debris flows produced an approximately symmetric debris-flow fan. In contrast, multigranular debris flows produced an asymmetric debris-flow fan, and the topography and range differed in each case. These results suggest that grain-size distributions of debris flows affect the process of debris-flow fan formation.