日本地球惑星科学連合2023年大会

講演情報

[J] 口頭発表

セッション記号 S (固体地球科学) » S-SS 地震学

[S-SS06] 地震発生の物理・断層のレオロジー

2023年5月23日(火) 09:00 〜 10:15 302 (幕張メッセ国際会議場)

コンビーナ:澤井 みち代(千葉大学)、金木 俊也(産業技術総合研究所)、奥脇 亮(筑波大学)、浦田 優美(産業技術総合研究所)、座長:浦田 優美(産業技術総合研究所)、奥脇 亮(筑波大学)


09:30 〜 09:45

[SSS06-03] Centroid moment tensor analysis of waveform data from ocean bottom seismometers by using 3-D seismic velocity structure

★Invited Papers

*山谷 里奈1 (1.防災科学技術研究所)


キーワード:セントロイド・モーメントテンソル、海底地震計

It is important to determine focal mechanisms of earthquakes for investigating stress fields in subduction zones. Stress changes after large earthquakes help understand the earthquake generation mechanisms and the state of mechanical coupling between the subducting and overriding plates. Tectonic stress fields and such stress changes have been estimated from stress orientations obtained from focal mechanisms (e.g., Terakawa and Matsu’ura, 2023). Increase of the spatial and temporal densities and resolutions of the focal mechanisms has a potential to increment those of the stress fields.

One of the ideas to obtain more focal mechanisms is to conduct centroid moment tensor inversion using waveform data from ocean bottom seismometers. Recently, ocean bottom seismometer networks of both temporary and permanent deployment have been developed along subduction zones (e.g., Cascadia Initiative: Toomey et al., 2014; DONET: Kaneda et al., 2015; S-net: Kanazawa et al., 2016.). However, most studies using short-period OBSs have only extracted information of the phase arrivals such as travel time and amplitude polarity. Recent developments of constructing 3-D high-resolution seismic velocity structure models and calculating synthetic waveforms using 3-D models enable us to analyze waveform data from ocean bottom seismometers (Yamaya et al., 2022), which have a potential to reveal tectonic stress field in subduction zones.