日本地球惑星科学連合2018年大会

講演情報

[EJ] Eveningポスター発表

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-CG59] 日本列島の構造と進化: 島弧の形成から巨大地震サイクルまで

2018年5月22日(火) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 7ホール)

コンビーナ:佐藤 比呂志(東京大学地震研究所地震予知研究センター)、篠原 雅尚(東京大学地震研究所)、石川 正弘(横浜国立大学大学院環境情報研究院、共同)、松原 誠(防災科学技術研究所)

[SCG59-P02] Spatial distribution of reflection intensity on the upper surface of the Philippine Sea Plate, off the Boso Peninsula, Japan

*河野 昭博1佐藤 利典1篠原 雅尚2望月 公廣2山田 知朗2植平 賢司3眞保 敬4町田 祐弥4日野 亮太5東 龍介5 (1.千葉大学大学院理学研究科地球生命圏科学専攻地球科学コース、2.東京大学地震研究所、3.防災科学技術研究所、4.海洋研究開発機構、5.東北大学大学院理学研究科)

キーワード:フィリピン海プレート、走時マッピング法、海底地震計、3次元P波速度構造、房総沖スロースリップイベント、伊豆小笠原マリアナ島弧

In the region off the Boso Peninsula, Japan, is known to have complex structure its underneath. The Pacific plate (PAC) is subducting westward beneath the landward plate from the Japan trench, while the Philippine Sea plate (PHS) is subducting northwestward under the landward plate from the Sagami trough. These complex tectonic interactions have caused various seismic events such as the Boso Slow Slip Events (SSEs). To better understand these seismic events, it is important to determine the structure under this region.

In May 2017, we published a 2D P-wave velocity structure under the survey area, showing geometry of the upper surface of PHS (UPHS) and reflection intensity variation along the UPHS. From our result and previous studies, relatively strong reflection from the UPHS can be observed near the main slip area of Boso SSEs. The reflective area may be related to the Boso SSEs, however, it is still insufficient to link both only from the 2D models. Therefore, further work is needed in order to reveal spatial distribution of the relatively strong reflection area.

From July to August 2009, we conducted a marine seismic experiment using airguns as sources off the southeast coast of the Boso Peninsula. Airguns were shot along the 4 survey lines and 27 Ocean Bottom Seismometers (OBSs) were deployed in the survey area. We used 18 OBSs to determine 3D P-wave velocity structure, which has 150(x)×90(y)×30 (z) km size.

We estimated 3D velocity structure from airgun data recorded in the OBSs by using the FAST (First Arrival Seismic Tomography; Zelt and Barton, 1998). We also picked the reflection traveltimes likely reflected from the UPHS and applied them to the Traveltime mapping method (Fujie et al. 2006) to estimate spatial locations of the reflectors.

As a result, the reflections from the UPHS seem to be concentrated in the western and the eastern part of the survey area. The western reflective area is close to the main slip area of the Boso SSEs, which may suggest the presence of a thin low velocity layer along the UPHS in the area. The eastern reflective area seems to overlap with the local high velocity structure seen in our 3D velocity structure. The high velocity structure partially overlaps with the northern extent of relatively high velocity structure seen in the forearc region of the Izu-Bonin subduction zone.