日本地球惑星科学連合2015年大会

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セッション記号 S (固体地球科学) » S-SS 地震学

[S-SS26] 地震波伝播:理論と応用

2015年5月26日(火) 14:15 〜 16:00 103 (1F)

コンビーナ:*齊藤 竜彦(独立行政法人 防災科学技術研究所)、中原 恒(東北大学大学院理学研究科地球物理学専攻固体地球物理学講座)、松島 潤(東京大学大学院)、西田 究(東京大学地震研究所)、白石 和也(株式会社地球科学総合研究所)、座長:志藤 あずさ(京都大学)、武村 俊介(横浜市立大学)

15:00 〜 15:15

[SSS26-15] Comparison between ray theory and synthetic seismograms for transversely isotropic media

*Anselme BORGEAUD1Kensuke KONISHI1Robert J. GELLER1Kenji KAWAI2 (1.Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo、2.Department of Earth Science and Astronomy, Graduate School of Arts and Sciences, University of Tokyo)

キーワード:DSM, Travel time, D double prime, Upper mantle, Anisotropy, S-wave splitting

Imaging seismic anisotropy is essential for a better understanding of geodynamics, since it provides information on deformation and flow in the crust and mantle. S-wave splitting has been widely used to infer the presence and extent of anisotropy. The inference of anisotropy from S wave splitting relies, however, on ray theory, which is strictly valid only for infinitely high frequencies, and thus may not accurately reflect real finite-frequency seismic data. For example, a recent study by Komatitsch et al. (2010) showed that splitting of diffracted S waves in the D'' region, just above the CMB, is present in synthetics computed for an isotropic velocity model. In this study we compute travel times for a transversely isotropic (TI) medium using a newly developed software package (Konishi et al., JpGU, 2015). We then compute full-wave synthetics using the Direct Solution Method (DSM; Kawai et al., 2006). We focus on two regions of the mantle: D'' and the upper mantle. We confirm apparent S-wave splitting in synthetics computed for the isotropic IASP91 velocity model for epicentral distances over 100 degrees, in agreement with the results of Komatitsch et al. (2010). We also compare the predictions of geometrical optics to synthetics for TI models for phases which sample the upper mantle and the D'' region.