作者
Paul Somerville,N. F. Smith,Robert Graves,Norman A. Abrahamson
摘要
Research Article| January 01, 1997 Modification of Empirical Strong Ground Motion Attenuation Relations to Include the Amplitude and Duration Effects of Rupture Directivity Paul G. Somerville; Paul G. Somerville Woodward-Clyde Federal Services 566 El Dorado Street Pasadena, CA 91101 e-mail: pgsomer0@wcc.com (P.G.S., N.F.S., R. W.G.) Search for other works by this author on: GSW Google Scholar Nancy F. Smith; Nancy F. Smith Woodward-Clyde Federal Services 566 El Dorado Street Pasadena, CA 91101 e-mail: pgsomer0@wcc.com (P.G.S., N.F.S., R. W.G.) Search for other works by this author on: GSW Google Scholar Robert W. Graves; Robert W. Graves Woodward-Clyde Federal Services 566 El Dorado Street Pasadena, CA 91101 e-mail: pgsomer0@wcc.com (P.G.S., N.F.S., R. W.G.) Search for other works by this author on: GSW Google Scholar Norman A. Abrahamson Norman A. Abrahamson Pacific Gas & Electric Co. Geosciences Dept. PO Box 770000 Mail Code N4C San Francisco, CA 94177 (N.A.A.) Search for other works by this author on: GSW Google Scholar Seismological Research Letters (1997) 68 (1): 199–222. https://doi.org/10.1785/gssrl.68.1.199 Article history first online: 09 Mar 2017 Cite View This Citation Add to Citation Manager Share Icon Share Twitter LinkedIn Tools Icon Tools Get Permissions Search Site Citation Paul G. Somerville, Nancy F. Smith, Robert W. Graves, Norman A. Abrahamson; Modification of Empirical Strong Ground Motion Attenuation Relations to Include the Amplitude and Duration Effects of Rupture Directivity. Seismological Research Letters 1997;; 68 (1): 199–222. doi: https://doi.org/10.1785/gssrl.68.1.199 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietySeismological Research Letters Search Advanced Search Abstract Rupture directivity effects cause spatial variations in ground motion amplitude and duration around faults and cause differences between the strike-normal and strike-parallel components of horizontal ground motion amplitudes, which also have spatial variation around the fault. These variations become significant at a period of 0.6 second and generally grow in size with increasing period. We have developed modifications to empirical strong ground motion attenuation relations to account for the effects of rupture directivity on strong motion amplitudes and durations. The modifications are based on an empirical analysis of near-fault data. The ground motion parameters that are modified include the average horizontal response spectral acceleration, the duration of the acceleration time history, and the ratio of strike-normal to strike-parallel spectral acceleration. The parameters upon which the adjustments to average horizontal amplitude and duration depend are the fraction of the fault rupture that occurs on the part of the fault that lies between the hypocenter and the site, and the angle between the fault plane and the path from the hypocenter to the site. Since both of these parameters can be derived from the hypocenter location and the fault geometry, the model of rupture directivity effects on ground motions that we have developed can be directly included in probabilistic seismic hazard calculations. The spectral acceleration is larger for periods longer than 0.6 second, and the duration is smaller, when rupture propagates toward a site. For sites located close to faults, the strike-normal spectral acceleration is larger than the strike-parallel spectral acceleration at periods longer than 0.6 second in a manner that depends on magnitude, distance, and angle. To facilitate the selection of time histories that represent near-fault ground motion conditions in an appropriate manner, we provide a list of near-fault records indicating the rupture directivity parameters that each contains. This content is PDF only. Please click on the PDF icon to access. First Page Preview Close Modal You do not have access to this content, please speak to your institutional administrator if you feel you should have access.