Rupture process of the 1995 Antofagasta subduction earthquake (Mw=8.1)

被引:19
作者
Carlo, DL [1 ]
Lay, T
Ammon, CJ
Zhang, JJ
机构
[1] Univ Calif Santa Cruz, Dept Earth Sci, Santa Cruz, CA 95064 USA
[2] St Louis Univ, Dept Earth Sci, St Louis, MO 63103 USA
关键词
finite-source rupture models; Chilean tectonics; seismic directivity;
D O I
10.1007/s000240050248
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
A finite-source rupture model of the July 30, 1995, M-w = 8.1 Antofagasta (Northern Chile) subduction earthquake is developed using body and surface waves that span periods from 20 to 290 s. A long-period (150-290 s) surface-wave spectral inversion technique is applied to estimate the average finite-fault source properties. Deconvolutions of broadband body waves using theoretical Green's functions, and deconvolutions of broadband fundamental mode surface waves using empirical Green's functions provided by a large aftershock, yield effective source time functions containing periods from 20 to 200 s for many directivity parameters. The source time functions are used in an inverse radon transform to image a one-dimensional spatial model of the moment rate history. The event produced a predominantly unilateral southward rupture, yielding strong directivity effects on all seismic waves with periods less than a few hundred seconds. The aftershock information, spectral analysis, and moment rate distribution indicate a rupture length of 180-200 km, with the largest slip concentrated in the first 120 km, a rupture azimuth of 205 degrees +/- 10 degrees along the Chilean coastline, and a rupture duration of 60-68 s with a corresponding average rupture velocity of 3.0-3.2 km/s. The overall rupture character is quite smooth, accentuating the directivity effects and reducing the shaking intensity, however there are three regions with enhanced moment rate distributed along the rupture zone: near the epicenter, 50 to 80 km south of the epicenter, and 110 to 140 km south of the epicenter.
引用
收藏
页码:677 / 708
页数:32
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