日本地球惑星科学連合2015年大会

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セッション記号 S (固体地球科学) » S-VC 火山学

[S-VC47] 火山・火成活動と長期予測

2015年5月26日(火) 11:00 〜 12:45 303 (3F)

コンビーナ:*及川 輝樹(独)産業技術総合研究所 活断層・火山研究部門)、長谷川 健(茨城大学理学部地球環境科学コース)、三浦 大助(財団法人電力中央研究所 地球工学研究所 地圏科学領域)、石塚 吉浩(産業技術総合研究所活断層・火山研究部門)、下司 信夫(産業技術総合研究所 地質情報研究部門)、座長:上木 賢太(独立行政法人海洋研究開発機構地球内部物質循環研究分野)、広井 良美(東北大学東北アジア研究センター)

11:45 〜 12:00

[SVC47-10] 遠方におけるラハール堆積物の堆積相変化‐鳥海火山の例‐

*南 裕介1大場 司2林 信太郎3片岡 香子4 (1.秋田大学大学院工学資源学研究科、2.秋田大学国際資源学部、3.秋田大学教育文化学部、4.新潟大学災害・復興科学研究所)

キーワード:ラハール, 鳥海火山

Chokai volcano is an andesitic stratovolcano in northeast Japan. The sector collapse of the volcano occurred about 2,500 years ago. The Kisakata debris avalanche deposit was formed by the collapse to the northern foot of Chokai volcano (Ohsawa et al., 1982). The post-collapse fan (partly volcaniclastic apron) deposits, largely distributed in the northern foot of the volcano, overlies the Kisakata debris avalanche deposit. From geological survey in the proximal area, Minami et al. (2015) reported that the post-collapse fan deposits accumulated by a series of debris flows and hyperconcentrated flows, and then concluded that the deposits are originated from several lahar events. However, change in sedimentary facies in the distal area was not well studied. Furthermore the depositional processes changes between the proximal and distal areas of these lahar deposits have not been well understood. This study aims to understand transition of depositional processes with distance, and relationship between geomorphology formed by these lahar deposits and their depositional processes. The volcanic fan can be topographically subdivided into four areas; the steeply-sloping area, the moderately-sloping area, the gently-sloping area, and the very-gently-sloping area. We trenched and cored (by handy geoslicer; Takada et al., 2002) in the distal of volcanic fan (gently sloping area, and very gently sloping area) at a total of 12 sites. Each set of trench and core by the depth of one to two meters from the surface were observed. In the distal area, the lahar deposits are composed of debris flow, hyperconcentrated flow and streamflow facies. These flows are mostly originated from lahar events. The facies variation with distance implies that lahars flowed down as debris flows in proximal areas. Then, they transformed into hyperconcentrated and stream flows, although some reached to the distal area as debris flow. Some lahar reached to the coastline that is 20 km distant from the volcanic edifice as stream flow, where highly populated towns are distributed.