日本地球惑星科学連合2024年大会

講演情報

[J] ポスター発表

セッション記号 S (固体地球科学) » S-SS 地震学

[S-SS05] 地震発生の物理・断層のレオロジー

2024年5月27日(月) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

コンビーナ:奥田 花也(海洋研究開発機構 高知コア研究所)、浦田 優美(産業技術総合研究所)、奥脇 亮(筑波大学)、澤井 みち代(千葉大学)


17:15 〜 18:45

[SSS05-P03] 波形インバージョン解の観測点分布依存性

*柴田 律也1麻生 尚文2,1 (1.東京工業大学理学院地球惑星科学系、2.東京理科大学先進工学部物理工学科)

キーワード:震源過程、波形インバージョン、経験的グリーン関数

Which source model is most realistic? This has been problematic in source kinematics for a long time. The difference in slip models can be due to the difference in the velocity structure, station selection, inversion setting, and methodology. Regarding the station selection, many studies have tried to use high-S/N waveforms with dense station coverage. Although such an effort is required to obtain more accurate slip models, the best way to choose stations has not been established.
In this study, we investigated the effect of the station selection on the waveform inversion results. We utilized the radiation-corrected empirical Green’s function (EGF; Shibata et al. 2022) in the inversion and compared the inversion results among several EGF events for each mainshock. The radiation correction was conducted with the theoretical ray parameter calculated by the TauP package (Crotwell et al. 1999) assuming the velocity structure of the JMA2001 (Ueno et al. 2002). The waveform inversion with the finite fault was performed as the multi-time-window method (Olson & Apsel 1982; Hartzell & Heaton 1983). As we used the trigger-type recordings of the KiK-net stations, operated by the National Research Institute for Earth Science and Disaster Prevention (Aoi et al. 2004), the available stations depended on the EGF events. In this regard, all the available stations within the epicentral distance of 100 km were utilized for the inversion with no arbitrary data selection. Although the waveforms of each EGF event have their own noise, we could estimate the effect of the station coverage by investigating multiple mainshocks.
As a result, we confirmed that the comprehensive characteristic of the slip image was commonly estimated among several EGF events in a case with a better waveform fitting than the variance reduction of 40.0%. In contrast, a subtle difference was confirmed on subfault scale, which can be caused by the station coverage. In addition, when we utilized the same station distribution between two EGF events, the slip images were closer than the original analyses with all the available stations.