English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 18076/20274 (89%)
造訪人次 : 5252330      線上人數 : 1320
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.cnu.edu.tw/handle/310902800/27762


    標題: A Rupture Model for the 1999 Chi-Chi Earthquake from Inversion of Teleseismic Data Using the Hybrid Homomorphic Deconvolution Method
    作者: Liao, Boi-Yee
    Sheu, Tian-Wei
    Yeh, Yeong-Tien
    Huang, Huey-Chu
    Yang, Lien-Shiang
    貢獻者: 應用空間資訊系
    關鍵字: Multichannel Blind Deconvolution
    Empirical Greens-Functions
    Source Time Functions
    Strong-Motion
    Cape Mendocino
    Seismic Data
    Body Waves
    Taiwan
    Fault
    Events
    日期: 2013-03
    上傳時間: 2014-05-26 10:42:38 (UTC+8)
    出版者: Springer Basel Ag
    摘要: This study investigates the kinematics of the rupture process of the M-L 7.3 Chi-Chi, Taiwan, earthquake on September 21, 1999. By applying the proposed hybrid homomorphic deconvolution method to deconvolve teleseismic broadband P-wave displacement recordings of the earthquake, this study derives the apparent source time functions (ASTFs) at ten stations located around the epicenter. To further characterize the fault, the kinematic history of the rupture was inverted from ASTFs using a genetic algorithm, coupled with nonlinear iterative technique. The calculated ASFTs reveal that the total rupture event lasted for approximately 27 s. Static slip distribution images indicate that most slip occurred at shallower portions of the fault plane, especially 20-55 km north of the epicenter. The maximum slip reached 20 m at 45 km north of the epicenter, and the average slip throughout the observed rupture area was approximately 2 m. Large asperities on the fault appeared at 25-35 km and 40-50 km north of the hypocenter, and coincided with relatively high rupture velocity. This suggests that the earthquake's energy may have been released quickly. The rupture velocity decreased upon encountering an asperity, and increased again after passing the asperity. This implies that the rupture required more time to overcome the resistances of the asperities. The maximum rupture velocity was 3.8 km/s, while the average rupture velocity was approximately 2.2 km/s. The rise time distribution suggests that larger slip amplitudes generally correspond to shorter rise times on the subfaults.
    關聯: Pure And Applied Geophysics, v.170 n.3, pp.391-407
    顯示於類別:[應用空間資訊系(所)] 期刊論文

    文件中的檔案:

    檔案 描述 大小格式瀏覽次數
    index.html0KbHTML2254檢視/開啟


    在CNU IR中所有的資料項目都受到原著作權保護.

    TAIR相關文章

    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library IR team Copyright ©   - 回饋