Mechanical Models Suggest Fault Linkage through the Imperial Valley, California, USA

被引:9
作者
Dorsett, Jacob H. [1 ]
Madden, Elizabeth H. [2 ]
Marshall, Scott T. [3 ]
Cooke, Michele L. [4 ]
机构
[1] Indiana Univ, Dept Earth & Atmospher Sci, 1001 East 10th St, Bloomington, IN 47405 USA
[2] Univ Brasilia, Inst Geociencias, Observ Sismol, BR-70910900 Brasilia, DF, Brazil
[3] Appalachian State Univ, Dept Geol & Environm Sci, 572 Rivers St, Boone, NC 28608 USA
[4] Univ Massachusetts, Dept Geosci, 611 N Pleast St, Amherst, MA 01003 USA
基金
美国国家科学基金会;
关键词
SAN-ANDREAS FAULT; EARTHQUAKE RUPTURE FORECAST; SUPERSTITION HILLS FAULT; SOUTHERN CALIFORNIA; SLIP RATES; LOS-ANGELES; COACHELLA VALLEY; SURFACE RUPTURE; UPLIFT PATTERNS; SALTON-TROUGH;
D O I
10.1785/0120180303
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
The Imperial Valley hosts a network of active strike-slip faults that comprise the southern San Andreas fault (SAF) and San Jacinto fault systems and together accommodate the majority of relative Pacific-North American plate motion in southern California. To understand how these faults partition slip, we model the long-term mechanics of four alternative fault networks with different degrees of connectivity through the Imperial Valley using faults from the Southern California Earthquake Center Community Fault Model version 5.0 (v.5.0). We evaluate model results against average fault-slip rates from the Uniform California Earthquake Rupture Model v.3 (UCERF3) and geologic slip-rate estimates from specific locations. The model results support continuous linkage from the SAF through the Brawley seismic zone to the Imperial and to the Cerro Prieto faults. Connected faults decrease surface strain rates throughout the region and match more slip-rate data. Only one model reproduces the UCERF3 rate on the Imperial fault, reaching the lower bound of 15 mm/yr. None of the tested models reproduces the UCERF3 preferred rate of 35 mm/yr. In addition, high-strain energy density rates around the Cerro Prieto fault in all models suggest that the UCERF3 preferred rate of 35 mm/yr may require revision. The Elmore Ranch fault-slip rate matches the UCERF3 rate only in models with continuous linkage. No long-term slip-rate data are available for the El Centro and Dixieland faults, but all models return less than 2 mm/yr on the El Centro fault and 3.5-9.6 mm/yr on the Dixieland fault. This suggests that the Dixieland fault may accommodate a significant portion of plate-boundary motion.
引用
收藏
页码:1217 / 1234
页数:18
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