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Both models were jointly inverted simultaneously from the near-source strong ground motion recordings, teleseismic P waves, long-period Rayleigh waves, GPS displacement vectors and InSAR line-of-sight displacement image. The deformations are mapped onto the fault with strike 140A degrees and dip 50A degrees to the southwest. The coseismic period here represents the first 10 s after the rupture initiation, when over 99 per cent of our total seismic moment (3.07 x 10(18) Nm) is already released in our preferred coseismic model. Most coseismic slip occurs in a small rupture area of approximately 16 km along strike and in a depth range of 3-10 km. The average slip is 0.45 m; peak slip reaches about 0.90 m. Our result reveals that L\u0027Aquila rupture has a lag of 0.6 s before it first propagates updip to break an asperity equivalent to an M-w 5.7. And then the rupture propagates along strike to break a large patch located about 8.0 km along strike and 4.0 km updip from the hypocentre. The weighted average of the rise time and slip velocity are 0.71 s and 0.77 m s(-1), respectively. Our estimate of radiated seismic energy is 1.67 x 10(13) J, yielding an energy to seismic moment ratio of 0.55 x 10(-5), considerably smaller than the global average for shallow earthquakes. The early post-seismic period here represents the time window from 10 s to about first day. During this period, our preferred post-seismic model has an accumulated seismic moment of 6.0 x 10(17) Nm, equivalent to an M-w of 5.8. The afterslip distribution features two separated high slip fault patches, locating either near the hypocentre or the region with peak coseismic slip. Their locations only partially overlap with the fault patches with significant afterslip after the first day. In particular, the slip distribution of the shallower patch is quantitatively consistent with the Amoruso and Crescentini\u0027 diffusive afterslip model. Therefore, the coseismic rupture of the 2009 L\u0027Aquila earthquake was following by a slow-slip event with significant moment release in first hour.", "subitem_description_language": "en", "subitem_description_type": "Other"}]}, "item_10001_publisher_8": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "OXFORD UNIV PRESS", "subitem_publisher_language": "en"}]}, "item_10001_relation_14": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_type_id": {"subitem_relation_type_id_text": "10.1093/gji/ggu241"}}]}, "item_10001_source_id_9": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "1365-246X", "subitem_source_identifier_type": "EISSN"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Tomoko E. 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  1. 防災科研関係論文

Coseismic and potential early afterslip distribution of the 2009 M-w 6.3 L'Aquila, Italy earthquake

https://nied-repo.bosai.go.jp/records/4685
https://nied-repo.bosai.go.jp/records/4685
cdb97db5-2ba6-4bd6-a87d-a61fe51ebdfb
Item type researchmap(1)
公開日 2023-03-30
タイトル
言語 en
タイトル Coseismic and potential early afterslip distribution of the 2009 M-w 6.3 L'Aquila, Italy earthquake
言語
言語 eng
著者 Tomoko E. Yano

× Tomoko E. Yano

en Tomoko E. Yano

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Guangfu Shao

× Guangfu Shao

en Guangfu Shao

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Qiming Liu

× Qiming Liu

en Qiming Liu

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Chen Ji

× Chen Ji

en Chen Ji

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Ralph J. Archuleta

× Ralph J. Archuleta

en Ralph J. Archuleta

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抄録
内容記述タイプ Other
内容記述 In view of significant discrepancy between the slip models of the 2009 April 6 L'Aquila, (Italy) earthquake based on seismic waveforms or geodetic data, a new inversion strategy is proposed to constrain the coseismic rupture model and early post-seismic afterslip model of this earthquake. Both models were jointly inverted simultaneously from the near-source strong ground motion recordings, teleseismic P waves, long-period Rayleigh waves, GPS displacement vectors and InSAR line-of-sight displacement image. The deformations are mapped onto the fault with strike 140A degrees and dip 50A degrees to the southwest. The coseismic period here represents the first 10 s after the rupture initiation, when over 99 per cent of our total seismic moment (3.07 x 10(18) Nm) is already released in our preferred coseismic model. Most coseismic slip occurs in a small rupture area of approximately 16 km along strike and in a depth range of 3-10 km. The average slip is 0.45 m; peak slip reaches about 0.90 m. Our result reveals that L'Aquila rupture has a lag of 0.6 s before it first propagates updip to break an asperity equivalent to an M-w 5.7. And then the rupture propagates along strike to break a large patch located about 8.0 km along strike and 4.0 km updip from the hypocentre. The weighted average of the rise time and slip velocity are 0.71 s and 0.77 m s(-1), respectively. Our estimate of radiated seismic energy is 1.67 x 10(13) J, yielding an energy to seismic moment ratio of 0.55 x 10(-5), considerably smaller than the global average for shallow earthquakes. The early post-seismic period here represents the time window from 10 s to about first day. During this period, our preferred post-seismic model has an accumulated seismic moment of 6.0 x 10(17) Nm, equivalent to an M-w of 5.8. The afterslip distribution features two separated high slip fault patches, locating either near the hypocentre or the region with peak coseismic slip. Their locations only partially overlap with the fault patches with significant afterslip after the first day. In particular, the slip distribution of the shallower patch is quantitatively consistent with the Amoruso and Crescentini' diffusive afterslip model. Therefore, the coseismic rupture of the 2009 L'Aquila earthquake was following by a slow-slip event with significant moment release in first hour.
言語 en
書誌情報 en : GEOPHYSICAL JOURNAL INTERNATIONAL

巻 199, 号 1, p. 23-40, 発行日 2014-10
出版者
言語 en
出版者 OXFORD UNIV PRESS
ISSN
収録物識別子タイプ EISSN
収録物識別子 1365-246X
DOI
関連識別子 10.1093/gji/ggu241
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