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-CG49] Integrative seismic and secondary hazard/risk assessment

2025年5月29日(木) 15:30 〜 17:00 201A (幕張メッセ国際会議場)

コンビーナ:岩城 麻子(防災科学技術研究所)、Gerstenberger Matthew(GNS Science, New Zealand)、Chan Chung-Han(Department of Earth Sciences, National Central University)、Chairperson:Matthew Gerstenberger(GNS Science, New Zealand)、Hung-Yu Wu(National Cheng Kung University)

16:15 〜 16:30

[SCG49-10] Time History-Based Probabilistic Seismic Hazard Analysis based on a Ground Motion Generative Model

*松本 雄馬1、八百山 太郎1、李 尚元1、糸井 達哉1 (1.東京大学)

キーワード:確率論的地震ハザード評価、地震動モデル、深層生成モデル

This study proposes a novel framework for probabilistic seismic hazard analysis (PSHA) based on the probability distribution of ground motion time-history data generated by a ground motion generative model.

In general, the exceedance probability of a ground motion intensity measure is evaluated in PSHA using predictions from ground motion models (GMMs). Such hazard analysis results are widely utilized for various purposes. However, in performance-based earthquake engineering (PBEE), exemplified by the PEER-PBEE framework, seismic performance evaluations based on dynamic response analyses of buildings are increasingly common, often requiring ground motion time-history data as the input seismic hazard.

Against this background, we have developed GMMs capable of directly modeling the probability distribution of ground motion time-history data using generative adversarial networks (GANs), a type of deep generative model. We refer to such a GMM as a ground motion generative model (GMGM). Our proposed GMGM evaluates the distribution of ground motion time-history data by incorporating its source, propagation path, and site characteristics, making it promising for PSHA applications.

We construct a GMGM using a method called StyleGAN2 and a strong-motion observed record database of crustal earthquakes in Japan. The constructed GMGM considers moment magnitude as the source characteristic, rupture distance as the propagation path effect, and the average shear-wave velocity in the top 30 m (Vs30) as the site characteristic. Subsequently, we propose a novel formulation of PSHA, where the PSHA integral is computed through Monte Carlo sampling using ground motion time-history data generated by the GMGM. Finally, a numerical experiment is conducted for a specific site and its surrounding active faults to demonstrate the proposed method. The PSHA results are presented and compared with those obtained using existing empirical GMMs, focusing on peak ground velocity, to discuss the validity of the proposed method.