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タイトル: Shear wave velocity structure at the Fukushima forearc region based on H/V analysis of ambient noise recordings by ocean bottom seismometers
著者: Farazi, Atikul Haque
Ito, Yoshihiro  kyouindb  KAKEN_id  orcid https://orcid.org/0000-0001-9484-9539 (unconfirmed)
Garcia, Emmanuel Soliman M
Lontsi, Agostiny Marrios
Sánchez-Sesma, Francisco José
Jaramillo, Aristoteles
Ohyanagi, Shukei
Hino, Ryota
Shinohara, Masanao
著者名の別形: 伊藤, 喜宏
大柳, 修慧
キーワード: Japan
Seismic noise
Crustal structure
Full H/V inversion
Shear-wave velocity
発行日: Jun-2023
出版者: Oxford University Press (OUP)
The Royal Astronomical Society
誌名: Geophysical Journal International
巻: 233
号: 3
開始ページ: 1801
終了ページ: 1820
抄録: This study presents the shear wave velocity (VS) structures of sedimentary sequences and a section of the upper crustal layer in the Fukushima forearc region of the Japan Trench subduction zone, which were obtained by analysing the horizontal-to-vertical (H/V) spectral ratios of ambient vibration records. The H/V curves were derived using 31 d of continuous seismic data from 3 broad-band and 16 short-period ocean bottom seismometer (OBS) stations. Using the broad-band data, H/V ratios from 0.01 to 10 Hz were derived, but the ratios below 0.1 Hz frequencies were unusually large and temporally unstable. Characterization of seismic noise energy from ∼1 yr of seismic data of three broad-band OBSs revealed variable and elevated energy conditions below 0.1 Hz due to typical long-period oceanic noise; we link these observations with the unstable H/V ratios below this frequency. Therefore, H/V analysis was performed in the frequency range of 0.1–10 Hz for both broad-band and short-period OBSs to obtain subsurface VS profiles. For the forward calculation of the H/V ratios in the inversion process, we used the recently developed ‘hvgeneralized’ method, which is based on the diffuse field assumption, and accounts for the water layer on top of stratified media. Moreover, available prior geological and geophysical information was utilized during the inversion of the H/V curves. We found that subsurface VS ranged from approximately 30 m s⁻¹ at the seabed to approximately 4900 m s⁻¹ at 7000 m below the sea floor (mbsf). Starting with the best model candidate at each OBS location, the effect of the water layer on the H/V curve in the deep ocean was investigated by comparing synthetic H/V curves with and without the water layer. The synthetic H/V analysis revealed that the water layer had a significant effect on H/V amplitudes at higher frequencies (>1 Hz), whereas comparatively little effect was observed at lower frequencies (<1 Hz). This study provides an empirical basis for H/V analysis using OBS data to determine VS down to several kilometres of sedimentary sequences to the upper crust with high-resolution.
著作権等: © The Author(s) 2023. Published by Oxford University Press on behalf of The Royal Astronomical Society.
This is an Open Access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
URI: http://hdl.handle.net/2433/284056
DOI(出版社版): 10.1093/gji/ggad028
出現コレクション:学術雑誌掲載論文等

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