三维光线追踪与有限频率断层扫描的比较

S. K. Suhardja, Yosua Hotmaruli Lumban Gaol, A. Abdullah, A. Nugraha, Z. Zulfakriza
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摘要

我们利用墨西哥西南部的远震到达时间进行了三维地震层析成像。墨西哥俯冲带是东太平洋上升的各个板块接近北美西部的古海沟时,影响古法拉龙板块的连续破碎事件的结果。该地区的复杂性与里维拉板块和科科斯板块两个俯冲洋板块的年龄、组成、收敛速度和俯冲倾角不同有关。在这项研究中,我们比较了三维射线追踪层析成像模型和有限频率层析成像模型。最后的模型显示了光线追踪和有限频率之间的振幅和模式差异。3D光线追踪模型生成了地幔快速速度结构的清晰图像。与使用一维有限频核相比,较深的板具有更强的相干性,且随深度的展宽较小。然而,尽管有限频率和三维射线追踪模型在振幅和模式上显示出一些差异,但模型的总体一致性支持Yang等人(2009)的解释,即墨西哥西南部正在发生板块回滚。射线追踪和有限频率理论结果之间的一种可能的不同解释涉及里维拉板块的深层结构。有限频率模型表明,里维拉板块在大约300公里的深度可以清晰地观测到,但在更深的深度就会消失。然而,3-D射线追踪模型显示400公里深度以下有一个清晰的快速度带,因此我们的模型不支持400公里深度以上的里维拉板块板块撕裂
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Comparison of 3-D Raytracing and Finite Frequency Tomography
We performed 3-D seismic tomography using teleseismic arrival time at Southwest Mexico. The Mexican subduction zone results from successive fragmentation events that affected the ancient Farallon plate as various segments of the East Pacific rise approached the paleo-trench off western North America. The complexity in this region is related to two subducting oceanic plates, the Rivera and Cocos plates, that have different ages, compositions, convergence velocities and subduction dip angles. In this study, we compared the 3-D raytracing tomography model with finite frequency tomography model.  Final models show the differences in amplitude and pattern between the raytracing and finite frequency. 3D raytracing models produced sharper images of fast velocity structures in the mantle. The deeper slabs are more coherent and show less broadening with depth than using 1D finite frequency kernels. However, although the finite frequency and 3-D ray tracing models show some differences in amplitude and pattern, the overall agreement of the models supports the interpretation of Yang et al. (2009) that slab rollback is occurring in South Western Mexico.  One possible different interpretation between the raytracing and finite frequency theory results concerns the deep structure of the Rivera slab. The finite frequency models show that the Rivera slab is clearly observable at a depth of about 300km but fades away at greater depths. However, the 3-D ray tracing model shows a clear fast velocity band down to a depth of 400 km and thus our model does not support a slab tear of the Rivera plate above 400 km depth
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