ヘイワード断層の地震動を予測するシミュレーション(Simulations predict ground motion for earthquakes on Bay Area’s Hayward fault)

2026-04-27 ローレンス・リバモア国立研究所(LLNL)

米ローレンス・リバモア国立研究所(LLNL)の研究チームは、カリフォルニア州ベイエリアのヘイワード断層で将来発生し得る地震について、高精度シミュレーションによる地震動予測を実施した。研究ではスーパーコンピュータを用いて断層破壊の進行や地下構造の影響を解析し、地域ごとの揺れの強さや継続時間を詳細に再現した。その結果、堆積盆地や都市部の地盤条件によって揺れが増幅される可能性が示され、特に人口密集地域では長周期地震動の影響が大きくなると予測された。これらの成果は、建築物の耐震設計、インフラ防災、緊急対応計画の高度化に役立つと期待される。また、物理ベースの地震モデルを活用することで、従来より現実的な災害想定が可能になり、地震リスク評価の精度向上にも寄与する。

ヘイワード断層の地震動を予測するシミュレーション(Simulations predict ground motion for earthquakes on Bay Area’s Hayward fault)
Ground motion simulation of a magnitude 7 earthquake on the Hayward fault using the Lawrence Berkeley National Laboratory-Lawrence Livermore National Laboratory Earthquake Simulation platform.

<関連情報>

破壊の指向性と波動伝播効果がシミュレーションされた地動に及ぼす影響の分析MW ヘイワード断層で発生した7つの地震 Analysis of Rupture Directivity and Wave Propagation Effects on Simulated Ground Motion for MW 7 Earthquakes on the Hayward Fault

Rie Nakata;Arben Pitarka;David McCallen;Houjun Tang;Camilo Pinilla‐Ramos
Seismological Research Letters  Published:March 17, 2026
DOI:https://doi.org/10.1785/0220250161

Abstract

As part of the San Andreas fault system, the seismically active Hayward fault is a major contributor to the significant earthquake hazard in the San Francisco Bay Area (SFBA). Accurate ground‐motion predictions for large earthquakes on this fault are essential, but challenges arise due to uncertainties in exactly how the fault will rupture in future earthquakes and how wave propagation effects caused by the highly heterogeneous subsurface geological structure will influence site‐dependent ground motions. This study investigates the combined influence of rupture kinematics and subsurface structure on ground motion, using simulated broadband seismograms for 50 rupture realizations of an MW 7 Hayward fault earthquake. Ground motions are generated within the physics‐based Earthquake Simulation fault‐to‐structure exascale computing framework and the Graves–Pitarka kinematic fault rupture generator. In addition to direct comparisons with empirical ground‐motion model (GMM) estimates, ensemble‐averaged ground‐motion intensities are used to isolate and assess source and wave path effects. We find that the local structure causes complex wave propagation and spatial variability not fully represented by the GMMs. Rupture directivity produces nearly symmetric amplification and deamplification along the fault, whereas large‐slip patches yield localized influences. Among these factors, the wave propagation effects account for the largest deviation from the GMM predictions. Moreover, they contribute differently across frequencies: directivity effects peak at intermediate frequencies (∼1.5 s), but basin amplification and large‐slip patch effects are most prominent at lower frequencies. This study contributes to a broader effort toward understanding key factors controlling ground‐motion variability in the SFBA and provides detailed constraints for the development of region‐specific, nonergodic GMMs.

1702地球物理及び地球化学
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