日本地球惑星科学連合2024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-IT14] 地球深部科学

2024年5月31日(金) 10:45 〜 12:15 コンベンションホール (CH-B) (幕張メッセ国際会議場)

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)、土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、石井 貴之(岡山大学惑星物質研究所)、飯塚 理子(早稲田大学教育学部理学科地球科学専修)、座長:石井 貴之(岡山大学惑星物質研究所)、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)、土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、飯塚 理子(早稲田大学教育学部理学科地球科学専修)

12:00 〜 12:15

[SIT14-11] Constraining thermal and chemical heterogeneity in D″ beneath Central America based on waveform inversion for 3-D S- and P-velocity structure

*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、最下部マントル、実体波、沈み込みスラブ

The lowermost mantle region (D″) just above the core-mantle boundary (CMB) is the thermal boundary layer of mantle convection and the boundary layer where the core-mantle interaction occurs. Estimating the thermal and chemical structures in D″ leads to a better understanding of the Earth’s thermal and chemical evolution. Therefore, it is necessary to infer the S- and P-velocity structures with comparable high (at least 100 km vertically) resolution using the same quality data and to distinguish thermal and chemical effects.
In this study, using the waveform inversion method, we try to infer the 3-D S- and P-velocity structures in D″ beneath Central America at a high resolution (~ 250 km horizontally and ~ 50 km vertically). We assembled a dataset of three waveform components from deep- and intermediate-focus South American, Caribbean, and Alaskan events mainly recorded at the full USArray network stations. Our preliminary model showed that we resolve S-velocity structures well in the whole parts of D″ thanks to the three-component data, suggesting the paleo-Farallon slab exists in the whole parts of D″. In contrast, we resolve the P-velocity structure in smaller areas than the S-velocity structure because of the paucity of available PcP data.
Sensitivity analysis demonstrated that the later half wavelength of the direct P-phase mainly contributes to the resolution of the P-velocity structure in D″. Therefore, we gather the additional waveform data from shallower and weaker events containing the direct P-phase in order to obtain a better resolution of the P-velocity structure. In the presentation, we will show the inversion results with additional data and the feasibility of the inversion using the direct P-phase with quantitative resolution tests and discuss their geophysical implication.