日本地球惑星科学連合2025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-CG 固体地球科学複合領域・一般

[S-CG45] Science of slow-to-fast earthquakes

2025年5月26日(月) 15:30 〜 17:00 国際会議室 (IC) (幕張メッセ国際会議場)

コンビーナ:加藤 愛太郎(東京大学地震研究所)、山口 飛鳥(東京大学大気海洋研究所)、中田 令子(東京大学大学院理学系研究科)、大久保 蔵馬(防災科学技術研究所)、座長:縣 亮一郎(海洋研究開発機構)、高木 涼太(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)

16:15 〜 16:30

[SCG45-10] Adjoint tomography of the Nankai and Kyushu subduction zones - Waveform misfits and assessment of existing 3D velocity models

*Samriddhi Prakash Mishra1Yoshihiro Kaneko1、Bryant Chow2Shun Adachi1Yusuke Yamashita3Masanao Shinohara4 (1.Graduate School of Science, Kyoto University、2.University of Alaska – Fairbanks, Alaska, USA、3.Disaster Prevention Research Institute, Kyoto University, Kyoto, Japan、4.Earthquake Research Institute, University of Tokyo, Tokyo Japan)


キーワード:seismic tomography , full waveform inversion, adjoint methods, subduction zones, Nankai Trough

The Nankai-Kyushu subduction system is a complex seismotectonic region marked by an abrupt transition in the inter-plate coupling, with a fully coupled megathrust to the northeast. In this study, we utilize an earthquake-based, full-waveform inversion technique, termed Adjoint Tomography (Tromp et al., 2005; Fichtner et al., 2006; Tape et al., 2007), to develop an accurate and high-resolution P-wave and S-wave velocity models of the Nankai-Kyushu subduction zone. We aim to reveal the crustal structure responsible for the origin of the inter-plate coupling transition. Our target region includes ~100 regional earthquakes (4.5 < Mw <6) with ~ 400 permanent receivers, DONET, and ~20 temporary Ocean Bottom Seismometers (OBS) stationed in the Hyuga-nada region. We first assess the accuracy of two candidate initial velocity models (Koketsu et al., 2012; Bassett et al., 2022). For the Bassett et al. (2022) model, we use empirical relations to convert P-wave velocities to obtain the corresponding S-wave velocity model. Using a spectral element solver, we simulate the earthquakes and compare the resulting synthetics with recorded waveforms at 6 – 40 s period ranges. Our results suggest that seismic waves are systematically amplified by accretionary sediments. We also perform a quantitative misfit analysis, incorporating parameters such as time shifts, amplitude ratios, peak cross-correlation, and apparent velocities. Our analysis reveals that large (> 3 s) travel-time misfits emerge in these initial models. Nevertheless, the overall time shifts and amplitude ratios, high peak cross-correlation values, and even distribution of phase measurements among components suggest that both models are reasonable starting models for computationally intensive adjoint tomography. We will present our ongoing efforts towards developing an updated velocity model of the study region that is more accurate and has higher resolution than the existing velocity models.