日本地球惑星科学連合2022年大会

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[E] 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-IT19] 地球深部科学

2022年5月22日(日) 15:30 〜 17:00 展示場特設会場 (2) (幕張メッセ国際展示場)

コンビーナ:太田 健二(東京工業大学理学院地球惑星科学系)、コンビーナ:河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)、飯塚 毅(東京大学)、コンビーナ:土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、座長:飯塚 毅(東京大学)、河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)

15:45 〜 16:00

[SIT19-08] Inferring 3-D S- and P-velocity structure of D″ beneath the Central America using waveform inversion

*佐藤 嶺1鈴木 裕輝2河合 研志1 (1.東京大学、2.東京工業大学)


D″, the lowermost layer of the Earth’s mantle, is one of the main regions which contain thermal or chemical composition anomalies and is important to understand the Earth’s thermal and chemical evolution. Two theories explaining the chemical evolution of D″ are mainly suggested; (i) chemical differentiation caused by partial melting at thermal boundary layer; (ii) mid ocean ridge basalt segregate from slabs and cumulate above the core-mantle boundary. Therefore, structure estimation at high-resolution, at least which can resolve subducted slabs; ~100km resolution, is required to search the factor of chemical composition anomaly. In order to distinguish thermal and chemical composition heterogeneity, it is necessary to infer the S- and P- velocity structure with comparable resolution using the same quality data. In this study, we expand waveform inversion to estimate S- and P-velocity structure simultaneously at high-resolution (horizontally ~250km and vertically ~100km). Then, we invert the USArray dataset for the 3-D S- and P-velocity structure of D″ beneath Central America. Furthermore, we introduce “mantle correction” to exclude the effect of the 3-D heterogeneous structure except for D″. We will show the inferred models and the result of resolution tests.