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Seismic mapping of shallow fault zones in the San Gabriel Mountains from the Los Angeles Region Seismic Experiment, southern California

机译:来自加利福尼亚南部洛杉矶地区地震实验的圣盖博山浅断层带的地震测绘

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During the Los Angeles Region Seismic Experiment (LARSE), a reflection/refraction survey was conducted along a profile (line 1) extending from Seal Beach, California, northeastward to the Mojave Desert and crossing the Los Angeles and San Gabriel Valley basins and San Gabriel Mountains. In most shot gathers from the southern and central San Gabriel Mountains, clear secondary arrivals are seen that merge, or appear to merge, with first arrivals at three locations, including the location of the Vincent thrust fault, an exposed late Mesozoic/early Cenozoic megathrust. These secondary arrivals are interpretable as reflections in the shallow crust (<5 km depth) from a concave-upward interface that projects to the surface in the north near the Vincent thrust fault, is offset in its central part at the San Gabriel fault tan old branch of the San Andreas fault), and terminates in the south at 1 to 2 km depth at the southern mountain front. The velocity structure above and below this interface strongly suggests it is the Vincent thrust fault: intermediate velocities (6.2 km/s), consistent with mylonites overlying the Vincent thrust fault, are observed above it; lower velocities (5.8 km/s), consistent with the Pelona Schist underlying the Vincent thrust fault, are observed below it. Problems arise, however, in attempting to match this reflector to the exposed Vincent thrust fault, which is seen in outcrops east of line 1. The Vincent thrust fault is shallower than the reflector in most places. An unmapped structure (steep fault, monocline, or thrust fault) is required between line 1 and the outcrops that either drops the Vincent thrust fault down to the depths of the reflector or repeats the Vincent thrust fault beneath line 1 in the footwall of another thrust fault. An alternative interpretation of the reflector is a deep greenstone horizon within the Pelona Schist, although this alternative is not favored by the velocity structure. [References: 20]
机译:在洛杉矶地区地震实验(LARSE)期间,沿着剖面(线1)进行了反射/折射调查,该剖面从加利福尼亚的锡尔比奇向东北延伸到莫哈韦沙漠,并穿过洛杉矶和圣盖博谷地盆地以及圣盖博山。在南部和中部圣加百利山的大部分射出带中,可以看到明显的次生来临与三个地方(包括文森特逆冲断层的位置,中生代/早新生代大推力裸露)的初次到达合并或似乎合并。 。这些次要到达可以解释为是从一个浅凹地壳(<5 km深度)中的反射,从一个向上凹进的界面反射到文森特逆冲断层附近的北部表面,在其中心部分被San Gabriel断层抵消了。圣安德烈亚斯断层的分支),并在南部山前终止于南部,深度为1至2 km。该界面上方和下方的速度结构强烈表明它是文森特逆冲断层:在其上方观察到中等速度(6.2 km / s),与覆盖文森特逆冲断层的my石一致。在其下方观察到较低的速度(5.8 km / s),与位于文森特逆冲断层之下的佩洛纳·史斯特岩一致。但是,在尝试使该反射器与裸露的文森特逆冲断层匹配时会出现问题,这在1号线以东的露头中可以看到。文森特逆冲断层在大多数地方比反射器浅。在1号线和露头之间需要一个未映射的结构(陡断层,单斜线或逆冲断层),该结构要么将Vincent逆冲断层降到反射器的深度,要么在另一条逆冲的下盘壁的1号线以下重复Vincent逆冲断层故障。反射器的另一种解释是在Pelona Schist内部深绿岩层,尽管速度结构并不支持这种选择。 [参考:20]

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