English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 94201/94201 (100%)
造訪人次 : 81563942      線上人數 : 3917
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library IR team.
搜尋範圍 查詢小技巧:
  • 您可在西文檢索詞彙前後加上"雙引號",以獲取較精準的檢索結果
  • 若欲以作者姓名搜尋,建議至進階搜尋限定作者欄位,可獲得較完整資料
  • 進階搜尋


    請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/103589


    題名: Evidence for non-self-similarity of microearthquakes recorded at a Taiwan borehole seismometer array
    作者: 馬國鳳;Lin, Yen-Yu;Ma, Kuo-Fong;Kanamori, Hiroo;Song, Teh-Ru Alex;Lapusta, Nadia;Tsai, Victor C.
    貢獻者: 地球科學學院地球科學學系
    日期: 2016-08-01
    上傳時間: 2026-04-23 11:33:25 (UTC+8)
    出版者: Oxford University Press;Oxford University Press (OUP)
    摘要: 摘要: We investigate the relationship between seismic moment M 0 and source duration tw of microearthquakes by using high-quality seismic data recorded with a vertical borehole array installed in central Taiwan. We apply a waveform cross-correlation method to the three-component records and identify several event clusters with high waveform similarity, with event magnitudes ranging from 0.3 to 2.0. Three clusters—Clusters A, B and C—contain 11, 8 and 6 events with similar waveforms, respectively. To determine how M 0 scales with tw , we remove path effects by using a path-averaged Q. The results indicate a nearly constant tw for events within each cluster, regardless of M 0, with mean values of tw being 0.058, 0.056 and 0.034 s for Clusters A, B and C, respectively. Constant tw , independent of M 0, violates the commonly used scaling relation ${t_w} \propto M_0^{1/3}$ . This constant duration may arise either because all events in a cluster are hosted on the same isolated seismogenic patch, or because the events are driven by external factors of constant duration, such as fluid injections into the fault zone. It may also be related to the earthquake nucleation size.
    出版者: Oxford University Press (OUP)
    出版日期: 2016-08-01
    出處: Geophysical Journal International, 2016-08, Vol.206 (2), p.757-773
    版權: The Authors 2016. Published by Oxford University Press on behalf of The Royal Astronomical Society. 2016
    識別號: ISSN: 0956-540X
    識別號: ISSN: 1365-246X
    識別號: EISSN: 1365-246X
    識別號: DOI: 10.1093/gji/ggw172
    顯示於類別:[地球科學學系] 期刊論文

    文件中的檔案:

    檔案 描述 大小格式瀏覽次數
    index.html0KbHTML22檢視/開啟


    在NCUIR中所有的資料項目都受到原著作權保護.

    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