中大學術數位典藏-NCU Institutional Repository-提供博碩士論文、考古題、期刊論文、研究計畫等下載:Item 987654321/104229
English  |  正體中文  |  简体中文  |  Items with full text/Total items : 94274/94274 (100%)
Visitors : 82911095      Online Users : 2227
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library IR team.
Scope Tips:
  • please add "double quotation mark" for query phrases to get precise results
  • please goto advance search for comprehansive author search
  • Adv. Search
    HomeLoginUploadHelpAboutAdminister Goto mobile version


    Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/104229


    Title: Spatio-temporal distribution of seismic moment release near the source area of the 2011 Tohoku-Oki earthquake
    Authors: 林靜怡;Lin, Jing-Yi;Wu, Wen-Nan
    Contributors: 地球科學學院地球科學學系
    Keywords: Earth and Environmental Science;Earth Sciences;Earthquakes;Geology;Geophysics/Geodesy;Seismic activity;Seismic hazard;Temporal distribution
    Date: 2012-01-01
    Issue Date: 2026-04-23 11:45:59 (UTC+8)
    Publisher: Springer International Publishing AG;Berlin/Heidelberg: Springer Berlin Heidelberg
    Abstract: 摘要: To understand the generation mechanism of the 2011 Tohoku-Oki earthquake, we analyzed the spatial and temporal distribution of the cumulative seismic moment (Σ M 0 ) for all earthquakes along the Japan Trench listed in the global centroid moment tensor catalog between January 1976 and November 2011. Three areas with distinct characteristics of Σ M 0 are identified: (1) in the 2011 Tohoku-Oki source area, the Σ M 0 released in the down-dip portion (≥30 km) was greater than that in the up-dip portion (<30 km) before the mainshock; (2) the Σ M 0 of the up-dip portion in the region where slow slip activity prevails is greater than that of the down-dip portion throughout the study period; (3) in the surroundings of the source area, where interplate coupling is relatively low and the largest foreshock occurred, values of Σ M 0 for the down-dip and up-dip portions are both intermediate. Our results show that a megathrust rupture could be generated by large accumulations of strain energy at the subduction interface, resulting from the differential strain energy released in the down-dip and up-dip portions during the interseismic interval. We propose that the variation pattern of Σ M 0 may offer spatial constraints for seismic hazard assessment in the future.
    其他題名: Earth Planet Sp
    出版者: Berlin/Heidelberg: Springer Berlin Heidelberg
    出版日期: 2012-01-01
    出處: Earth, planets, and space, 2012-01, Vol.64 (12), p.1067-1075
    資源來源: Publicly available content database
    版權: The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences; TERRAPUB. 2012
    版權: The Society of Geomagnetism and Earth, Planetary and Space Sciences, The Seismological Society of Japan 2012
    識別號: ISSN: 1343-8832
    識別號: ISSN: 1880-5981
    識別號: EISSN: 1880-5981
    識別號: DOI: 10.5047/eps.2012.04.006
    Appears in Collections:[Department of Earth Sciences ] journal & Dissertation

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML15View/Open


    All items in NCUIR are protected by copyright, with all rights reserved.

    社群 sharing

    ::: Copyright National Central University. | 國立中央大學圖書館版權所有 | 收藏本站 | 設為首頁 | 最佳瀏覽畫面: 1024*768 | 建站日期:8-24-2009 :::
    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library IR team Copyright ©   - 隱私權政策聲明