論文

査読有り
2016年5月

Possible scenarios for occurrence of M similar to 7 interplate earthquakes prior to and following the 2011 Tohoku-Oki earthquake based on numerical simulation

SCIENTIFIC REPORTS
  • Ryoko Nakata
  • ,
  • Takane Hori
  • ,
  • Mamoru Hyodo
  • ,
  • Keisuke Ariyoshi

6
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1038/srep25704
出版者・発行元
NATURE PUBLISHING GROUP

We show possible scenarios for the occurrence of M similar to 7 interplate earthquakes prior to and following the M similar to 9 earthquake along the Japan Trench, such as the 2011 Tohoku-Oki earthquake. One such M similar to 7 earthquake is so-called the Miyagi-ken-Oki earthquake, for which we conducted numerical simulations of earthquake generation cycles by using realistic three-dimensional (3D) geometry of the subducting Pacific Plate. In a number of scenarios, the time interval between the M similar to 9 earthquake and the subsequent Miyagi-ken-Oki earthquake was equal to or shorter than the average recurrence interval during the later stage of the M similar to 9 earthquake cycle. The scenarios successfully reproduced important characteristics such as the recurrence of M similar to 7 earthquakes, coseismic slip distribution, afterslip distribution, the largest foreshock, and the largest aftershock of the 2011 earthquake. Thus, these results suggest that we should prepare for future M similar to 7 earthquakes in the Miyagi-ken-Oki segment even though this segment recently experienced large coseismic slip in 2011.

リンク情報
DOI
https://doi.org/10.1038/srep25704
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000375489600001&DestApp=WOS_CPL
Scopus
https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84966421185&origin=inward 本文へのリンクあり
Scopus Citedby
https://www.scopus.com/inward/citedby.uri?partnerID=HzOxMe3b&scp=84966421185&origin=inward
ID情報
  • DOI : 10.1038/srep25704
  • ISSN : 2045-2322
  • eISSN : 2045-2322
  • SCOPUS ID : 84966421185
  • Web of Science ID : WOS:000375489600001

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