日本地球惑星科学連合2023年大会

講演情報

[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-IT16] 地球深部科学

2023年5月25日(木) 10:45 〜 12:00 302 (幕張メッセ国際会議場)

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)、太田 健二(東京工業大学理学院地球惑星科学系)、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)、座長:土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、太田 健二(東京工業大学理学院地球惑星科学系)

11:45 〜 12:00

[SIT16-05] Constraining 3-D S- and P-velocity structure of D″ beneath the Central America from multiple component data using waveform inversion

*佐藤 嶺1河合 研志1 (1.東京大学大学院理学系研究科地球惑星科学専攻)


キーワード:波形インバージョン、D″領域、マントル最深部、実体波、沈み込みスラブ

D″, the lowermost layer of the Earth’s mantle, is one of the main regions which contain thermal or chemically compositional 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 the thermal boundary layer; (ii) mid-ocean ridge basalt (MORB) segregates from slabs and cumulates above the core-mantle boundary. Therefore, structure estimation at a high resolution, at least which can resolve in the D″ region, vertically ~100km resolution, is required to search the factor of chemical anomalies. In order to distinguish thermal and chemical effects, it is necessary to infer the S- and P- velocity structure with comparable resolution using the same quality data.
In this study, aiming to infer S- and P-velocity structure simultaneously at a high resolution (horizontally ~250km and vertically ~50km), we first conduct localized waveform inversion using transverse (T) and vertical (Z) components of the waveforms from South American, Caribbean, and Alaskan events recorded at the full USArray network stations and estimate the 3-D S-velocity structure in D″ beneath Central America. The inversion results show that we improve the resolution of the S-velocity structure, especially in the shallower part of D″ with two components. Second, we extend the waveform inversion method and try to constrain both 3-D S- and P-velocity structures using the same dataset. Our results indicate that we can resolve the P-velocity structure in the region densely sampled by P-wave. Our inferred models suggest the existence of the paleo-Farallon slabs and the Fe, Al-rich regions in which piles of the MORB may form. To enhance the resolution of the P-velocity structure, we improve the dataset. Our presentation will show the results with the improved data.