日本地球惑星科学連合2014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-CG66_30AM1] プレート収束帯における地殻変形運動の統合的理解

2014年4月30日(水) 09:00 〜 10:45 414 (4F)

コンビーナ:*深畑 幸俊(京都大学防災研究所)、八木 勇治(国立大学法人 筑波大学大学院 生命環境系)、鷺谷 威(名古屋大学減災連携研究センター)、橋本 学(京都大学防災研究所)、宍倉 正展(産業技術総合研究所 活断層・地震研究センター)、吉岡 祥一(神戸大学都市安全研究センター)、池田 安隆(東京大学大学院理学系研究科地球惑星科学専攻)、木村 学(東京大学大学院理学系研究科地球惑星科学専攻)、松浦 充宏(情報・システム研究機構 統計数理研究所)、座長:深畑 幸俊(京都大学防災研究所)、北 佐枝子(独立行政法人 防災科学技術研究所)

09:15 〜 09:30

[SCG66-02] 北海道下の3次元減衰構造:島弧-島弧衝突とM7 クラス内陸大地震(その3)

*北 佐枝子1中島 淳一2長谷川 昭2内田 直希2岡田 知己2勝俣 啓3浅野 陽一1木村 武志1 (1.防災科学技術研究所、2.東北大学大学院理学研究科附属地震・噴火予知研究観測センター、3.北海道大学大学院理学研究院附属地震火山研究観測センター)

キーワード:地震波減衰構造, 地震テクトニクス, 島弧衝突過程, スラブ内地震の応力降下量

1. IntroductionIn the Hokkaido corner, the Kuril fore-arc sliver collides with the northeastern Japan arc. Using travel-time data compiled from the nationwide Kiban seismic network and a dense temporary seismic network [Katsumata et al, 2002], Kita et al. [2012] determined high-resolution 3D seismic velocity structure beneath this area for deeper understanding of the collision process of the two fore-arcs. In this study, we merged waveform data from the Kiban-network and from the temporary network, and estimated the seismic attenuation structure to understand seismotectonics and collision process beneath Hokkaido. 2. Data and methodWe estimated corner frequency for each earthquake by the spectral ratio method of coda waves [e.g. Mayeda et al., 2007]. Then, we simultaneously determined values of t* and the amplitude level at low frequencies from the observed spectra after correcting for the source spectrum. Seismic attenuation (Q-1 value) structure was obtained, inverting t* values and employing the 3-D ray-tracing technique of Zhao et al. [1992]. The study region covers an area of 41-45N, 140.5-146E, and a depth range of 0-300 km. We obtained 154,293 t* at 316 stations from 6,196 events (Mj>2.0) that occurred during the period from Aug. 1999 to Dec. 2012. Horizontal and vertical grid nodes were set with spacing of 0.1-0.3 degrees and 10-30 km, respectively.3. ResultsThe calculated stress drops are distributed from 0.1 to 100 MPa. Stress drops of intraslab earthquakes increase with focal depth. The values of stress drops of events in the slab mantle tend to be larger than those in the slab crust at depths of 80 to 170 km, which might contribute to understanding of the physical nature of intraslab earthquakes.Seismic attenuation structure is imaged for the region above the subducting Pacific slab at depths down to ~80 km. For the forearc side of the eastern and western parts of Hokkaido, high-Qp zones are generally imaged at depths of 10 to 80 km in both the crust and mantle wedge above the Pacific slab. In contrast, low-Qp zones are clearly imaged in the mantle wedge of the backarcside.They are distributed in deeper parts and reach the Moho beneath the volcanic front. Locations of these low-Qp zones correspond to the low-Vp and low-Vs zones imaged by Zhao et al. [2012]. These suggest that the upper head of the mantle-wedge upwelling flow is detected beneath Hokkaido also by our seismic attenuation imaging.In the Hokkaido corner, to the west of the Hidaka main thrust a broad low-Qp zone is imaged at depths of 0?60 km. Location of this broad low-Qp zone almost corresponds to that of the low-V zone in the collision zone found by Kita et al. [2012]. Fault planes of the 1970 M6.7 and 1982 M7.1 earthquakes are located at the edges of a broad low-Qp zone, being in contact with a high-Qp zone at 10 to 35 km. These results suggest that the occurrence of these anomalously deep and large inland earthquakes is related to the presence of hydrous minerals or fluids.The subducting oceanic crust beneath the Hidaka region is imaged as a low-Q zone whose location corresponds to the low-Vp and low-Vs zone of Kita et al. [2012], suggesting the existence of hydrated materials at the top of the slab. Just above the slab surface, moderately low-Q zones are imaged at depths of 90 to 100 km beneath eastern and southern Hokkaido and at depths of 110 to 130 km beneath the corner, which are located at depths deeper than the upper plane seismic belt. These observations suggest the existence of the hydrated mantle wedge by the aqueous fluids supplied from the oceanic crust right below.