加利福尼亚长滩密集阵列的地震可探测性和深度分辨率:大陆环境下上地幔地震的进一步证据

A. Inbal, J. Ampuero, Robert W. Clayton
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摘要

新港-英格尔伍德断层(NIF)是一个缓慢变形的断层,穿过薄薄的大陆地壳,地热正常;但它却承载着南加州一些最深的地震。在这样的大陆环境中发生深层地震的成核原因尚不十分清楚。此外,深成震带意味着 NIF 地震的最大震级可能比预期的要大。在此,我们对用于研究 NIF 深层地震的长滩(LB)和扩展长滩(ELB)密集阵列的分辨率进行了量化。以前对区域目录和向下连续的长滩阵列数据的研究发现,NIF地震延伸到长滩阵列下方的上地幔。后来的研究分析了 ELB 原始数据,却几乎没有发现此类深层事件的证据。为了解决这一不一致问题,我们通过分析下移前和下移后的枸杞地震图和基准测试,对阵列的微地震可探测性和分辨能力进行了量化。向下迁移可将能量集中到震源区域,并消除地表噪声,从而显著提高可探测性和分辨率。随着阵列孔径与震源深度比的增加,可探测性也得到了提高。LB 阵列的最大孔径只比 ELB 阵列的孔径大 20%,但它对深度(>20 公里)事件的分辨率却提高了约 2 倍,这表明阵列几何形状的微小变化就能显著提高分辨率。假设孔径不变,我们发现 LB 阵列在使用 1%的传感器进行反投影时仍能保持分辨率。然而,高传感器密度对于提高信噪比至关重要。对区域和阵列得出的 NIF 目录以及新获得的 NIF 下方莫霍深度的分析表明,LB 下方的地幔地震可能是该断层的一个长期特征。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Earthquake Detectability and Depth Resolution with Dense Arrays in Long Beach, California: Further Evidence for Upper-Mantle Seismicity within a Continental Setting
The Newport–Inglewood fault (NIF) is a slowly deforming fault cutting through a thin continental crust with a normal geothermal; yet it hosts some of the deepest earthquakes in southern California. The nucleation of deep earthquakes in such a continental setting is not well understood. Moreover, the deep seismogenic zone implies that the maximum NIF earthquake magnitude may be larger than expected. Here, we quantify the resolution of the Long Beach (LB) and the Extended Long Beach (ELB) dense arrays used to study deep NIF seismicity. Previous study of the regional catalog and of downward-continued LB array data found NIF seismicity extending into the upper mantle beneath LB. Later studies, which analyzed the ELB raw data, found little evidence for such deep events. To resolve this inconsistency, we quantify the array’s microearthquake detectability and resolution power via analysis of pre- and postdownward migrated LB seismograms and benchmark tests. Downward migration focuses energy onto the source region and deamplifies the surface noise, thus significantly improving detectability and resolution. The detectability is also improved with the increase in the array aperture-to-source-depth ratio. The LB array maximum aperture is only 20% larger than the ELB aperture, yet its resolution for deep (>20 km) events is improved by about a factor of two, suggesting that small changes to the array geometry may yield significant improvement to the resolution power. Assuming a constant aperture, we find the LB array maintain resolution with 1% of its sensors used for backprojection. However, the high-sensor density is essential for improving the signal-to-noise ratio. Analysis of the regional and array-derived NIF catalogs together with newly acquired Moho depths beneath the NIF suggests that mantle seismicity beneath LB may be a long-lived feature of this fault.
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