日本地球惑星科学連合2019年大会

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セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG53] 活断層による環境形成・維持

2019年5月30日(木) 10:45 〜 12:15 A05 (東京ベイ幕張ホール)

コンビーナ:小泉 尚嗣(滋賀県立大学環境科学部)、山野 誠(東京大学地震研究所)、笠谷 貴史(海洋研究開発機構)、濱元 栄起(埼玉県環境科学国際センター)、座長:小泉 尚嗣後藤 忠徳(京都大学大学院工学研究科)

11:15 〜 11:30

[SCG53-03] 海域の断層近傍における熱流量異常に基づく流体流動の推定

*山野 誠1後藤 秀作2川田 佳史3濱元 栄起4 (1.東京大学地震研究所、2.産業技術総合研究所、3.東北大学災害科学国際研究所、4.埼玉県環境科学国際センター)

キーワード:熱流量異常、流体流動、断層、熱輸送、長期計測

Active fluid flow along faults may yield temperature or surface heat flow anomalies because advective heat transport by fluid flow is much more efficient than conductive transport. On land, it is rather difficult to observe such anomalies as temperature profile measurement in deep boreholes is required. On the other hand, we can conduct dense heat flow measurements on seafloor if surface sediment is soft enough to allow penetration of temperature probes. Heat flow and/or temperature anomalies in the vicinity of faults have been reported in some accretionary prisms, e.g., Cascadia and Barbados subduction zones. In this presentation, we show examples of heat flow anomalies associated with faults on the seafloor in the Nankai Trough area.
Accretionary prism developed landward of the Nankai Trough is extensively faulted in a compressional stress field due to subduction of the Philippine Sea plate. At the toe of the prism off Muroto, eastern Shikoku, closely-spaced heat flow measurements were made with a ROV and conspicuous high anomalies were found around the second frontal thrust, indicating that pore fluid flows upward along the fault (Kawada et al., 2014). Off the Kii peninsula, a large thrust fault system termed the megasplay cuts through the entire prism and its branches reach the seafloor. Yamano et al. (2014) conducted heat flow measurements with a surface ship across a branch of the megasplay and observed high heat flow values on the lower part of a fault scarp. Goto et al. (2008) made measurements with a submersible around biological communities along another branch of the megasplay and showed a sharp heat flow variation in a scale of several meters. These observations demonstrate that fluid flow along faults in various spatial scales can be detected by surface heat flow measurements.
The velocity or flux of vertical fluid flow may be estimated through long-term monitoring of temperature distribution in surface sediment. Temporal variation of the bottom water temperature propagates downward through sediment by thermal diffusion. Since this propagation process is affected by vertical fluid flow, analysis of long-term record of temperatures at multiple depths allows us to estimate fluid flow velocity (Goto et al., 2005). This method was applied to temperature records obtained in and around a biological community located a tip of the megasplay branch fault and the result indicates the existence of upward fluid flow (Kawada et al., 2013).