日本地球惑星科学連合2018年大会

講演情報

[EE] ポスター発表

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-IT22] 核-マントルの相互作用と共進化

2018年5月22日(火) 10:45 〜 12:15 ポスター会場 (幕張メッセ国際展示場 7ホール)

コンビーナ:飯塚 毅(東京大学)、渋谷 秀敏(熊本大学大学院先端科学研究部基礎科学部門地球環境科学分野)、土屋 卓久(愛媛大学地球深部ダイナミクス研究センター、共同)、太田 健二(東京工業大学大学院理工学研究科地球惑星科学専攻)

[SIT22-P13] A preliminary model for S-wave velocity structure in the D" region beneath New Guinea by using Thai Seismic Array (TSAR)

*田中 聡1W. Siripunvaraporn2S. Boonchaisuk2S. Noisagool2河合 研志3鈴木 裕輝3石原 靖4Taewoon Kim4宮川 幸治5竹内 希5川勝 均5 (1.海洋研究開発機構 地球深部ダイナミクス研究分野、2.マヒドン大学 理学部、3.東京大学 理学系研究科、4.海洋研究開発機構 地震津波海域観測研究開発センター、5.東京大学 地震研究所)

キーワード:Thai Seismic Array、D" layer

The edge of a Large-Low Shear Velocity Province (LLSVP) is an interesting area to understand active interaction with ambient mantle. To address such an issue, Thai Seismic Array (TSAR) has been constructed, which locates at an appropriate position to investigate the seismic structure in the D" region beneath New Guinea, where is the western edge of the Pacific LLSVP, by using deep earthquakes occurred in Fiji Islands. To date, we observed S, SKS, and ScS phases from deep Fiji earthquakes with distance range from 84° to 91°. The best event was occurred on Feb 24, 2017. After applying bandpass filter (0.04 – 0.3 Hz) and the correction of SKS splitting, the travel time differences of S–SKS, and ScS–SKS were measured on the radial components of velocity seismograms by picking the corresponding peaks and compared with those measured on reflectivity synthetic seismograms for PREM (Dziewonski and Anderson, 1981). The residuals of ScS–SKS differential travel times were +2 to +3 s, which were consistent with those predicted by the 3D model S40RTS (Ritsema et a., 2011). However, the residuals of S–SKS were about –3 s at shorter distances to 0 s at larger distances, which was not consisted with S40RTS. These observations suggest that a high velocity layer is imbedded in a low velocity region near the base of the mantle. Therefore, we conducted forward modeling using the waveforms to seek for the most appropriate structure. We considered velocity structures that were modified from PREM. S-wave velocity was assumed to linearly decrease from 2300 km depth up to several hundred km above the core-mantle boundary (CMB). To explain the S–SKS residual of 0 s at larger distances, we assumed that the reduction of S-wave velocity just above the velocity discontinuity was a half of the assumed velocity jump, then the velocity discontinuously increased by the assumed velocity jump. The S-wave velocity below the discontinuity (corresponding to the top of the D" layer) linearly increased or decreased to be the assumed value at the CMB. Here we prepared approximately 400 models for the thickness of D" layer to be 50 to 350 km with a 50km interval, the velocity jumps from 0.5 to 4.5% with a 0.5 % interval, and S wave velocity at the CMB from 7.0 to 7.4 km/s with a 0.05 km/s interval. By forward modeling with reflectivity synthetics, we obtained that the most preferred model has 4% velocity jump at 200 km above the CMB with Vs of 7.0 km at the CMB.