日本地球惑星科学連合2016年大会

講演情報

インターナショナルセッション(ポスター発表)

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT08] Structure and Dynamics of Suboceanic Mantle

2016年5月24日(火) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

コンビーナ:*是永 淳(イェール大学地球科学科)、川勝 均(東京大学地震研究所)、Gaherty James(Lamont Doherty Earth Observatory)、馬場 聖至(東京大学地震研究所)

17:15 〜 18:30

[SIT08-P03] Anisotropy in the Northwest Pacific oceanic lithosphere inferred from Po/So waves

*志藤 あずさ1末次 大輔2古村 孝志3塩原 肇3一瀬 建日3杉岡 裕子4伊藤 亜妃2竹尾 明子3歌田 久司3 (1.九州大学 大学院理学研究院附属 地震火山観測研究センター、2.海洋研究開発機構 地球深部ダイナミクス研究分野、3.東京大学 地震研究所、4.神戸大学 理学研究科 惑星学専攻)

キーワード:Po/So waves, anisotropy, oceanic lithosphere

Po/So waves, which have a high frequency, large amplitude, and long duration, propagate for large distances across oceanic lithosphere. These waves are generated by multiple forward scattering of P- and S-waves due to small-scale heterogeneities in oceanic lithosphere and P-waves trapped in seawater. To study the origin of such small-scale heterogeneities, we analyzed the azimuthal anisotropy of Po/So waves propagating in the Northwest Pacific.

Seismological observations using Broad Band Ocean Bottom Seismometers (BBOBSs) were conducted in the Northwest Pacific from 2010 to 2014 as a part of the Normal Oceanic Mantle Project. During the experiments, high-quality Po/So waves were recorded from earthquakes in the subducting Pacific plate. We determined travel times of the Po/So waves using an auto-picking algorithm based on an AR model, and estimated the average velocities of the Po/So waves between sources and stations. The average velocities of the Po/So waves traveling in the Northwest Pacific show clear variations as a function of azimuth, as follows:
VPo = 8.25 + 0.20 cos2(x − 153),
VSo = 4.71 + 0.04 cos2(x − 159).
The magnitudes of the anisotropy for Po and So waves velocities are 2.4% and 0.8%, respectively, which are smaller than the results of previous studies for Pn and Sn waves [Shimamura, 1984; Shinohara et al., 2008]. The fast direction is parallel to the past spreading direction of oceanic crust as estimated from magnetic anomalies [Nakanishi et al., 1992], which is roughly consistent with the previous studies [Shimamura, 1984; Shinohara et al., 2008].

We investigate the mechanism of the azimuthal anisotropy of Po/So wave propagation, which should be relating to the generation and evolution of the oceanic lithosphere using a Finite Difference Method (FDM) simulation of seismic wave propagation. We compare observed and calculated Po/So waves, and discuss the mechanism of their azimuthal anisotropy.