日本地球惑星科学連合2014年大会

講演情報

口頭発表

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-IT39_2AM2] 地球深部ダイナミクス:プレート・マントル・核の相互作用

2014年5月2日(金) 11:00 〜 12:45 416 (4F)

コンビーナ:*綿田 辰吾(東京大学地震研究所海半球観測研究センター)、境 毅(愛媛大学地球深部ダイナミクス研究センター)、中川 貴司(海洋研究開発機構地球内部ダイナミクス領域)、座長:河合 研志(東京工業大学大学院理工学研究科地球惑星科学専攻)

12:15 〜 12:30

[SIT39-P02_PG] Hi-netで計測される日本列島におけるsplitting intensity の空間的変化について II

ポスター講演3分口頭発表枠

*小川 直人1川勝 均1竹内 希1汐見 勝彦2 (1.東京大学 地震研究所、2.防災科学技術研究所)

キーワード:地震波異方性

To systematically investigate the spatial variation of seismic anisotropy around the Japanese islands, we measured the splitting intensity (SI) of teleseismic SKS and SKKS phases by Hi-net (Ogawa et al., 2013, SSJ). SI is first introduced by Chevrot (2000) as a method of measuring seismic anisotropy; it is based on cross-correlation of polarized waveforms, and can be modeled like the delay time of seismic tomography considering the effect of finite frequency (e.g., Favier and Chevrot, 2003). In this study, we extend our previous work by measuring SI for a large number of dataset recorded by the dense seismic station network, Hi-net. We use data from tilt-meters of Hi-net from October in 2000 to September in 2013. We have selected the recordings of SKS phases for epicentral distances between 90 and 135 degrees and SKKS beyond 105 degrees, and Mw larger than 6.0, resulting in a total number of events to be 189 that is much larger than the previous case. For the actual analysis, we apply a band-pass filter between 0.05 and 0.125 Hz, and the measurement error of each SI will be carefully estimated using a new formulation, as there appears an error in the Chevrot (2000)'s original treatment. The preliminary analysis indicates regional scale variations of SI patterns that apparently depend on the back azimuth of seismic event, which may be influenced by the subducting slabs.