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首页> 外文期刊>Pure and Applied Geophysics >Uppermost Inner Core Heterogeneity from Differential Travel Times of PKIKP vs. PKP-Bdiff and PKP-Cdiff Phases
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Uppermost Inner Core Heterogeneity from Differential Travel Times of PKIKP vs. PKP-Bdiff and PKP-Cdiff Phases

机译:PKIKP 与 PKP-Bdiff 和 PKP-Cdiff 相差差行程时间的最上层内核异质性

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摘要

We evaluate the average P-wave velocity perturbations of the Earth's uppermost inner core (IC) by analyzing two pairs of core phases: PKIKP-PKP-Bdiff (456 observations in the distance range of 138.5A degrees-142A degrees) and PKIKP-PKP-Cdiff (1215 observations at 155A degrees-162A degrees). The former is most sensitive to inner core velocities in the depth range of 350-590 km and the latter from 0 to 100 km below the inner core boundary. The differential travel-time residuals exhibit the roughly "east-west" hemispheric pattern especially beneath the Pacific Ocean. Here, the separation between the two quasi-hemispheres is near the 150A degrees W meridian (from PKP-Bdiff observations), but possibly rotated toward a NW-SE orientation, from PKP-Cdiff. Alternately, a velocity heterogeneity could be present here, in agreement with the previously reported PKIKP vs. PKPBC observations. Assuming the conventional definition for the IC quasi-hemispheres (i.e., the QEH between 0A degrees and 180A degrees E, and the QWH between 0A degrees and 180A degrees W), the quasi-Eastern hemisphere exhibits perturbations of (+1.17 +/- 0.04) (from PKIKP-PKP-Bdiff) and (+0.19 +/- 0.01) (from PKIKP-PKP-Cdiff). The corresponding perturbations in the quasi-Western hemisphere are of (-0.06 +/- 0.06) and (-0.19 +/- 0.02) , respectively. An anomalous IC zone beneath the Indian Ocean is not conspicuous in our PKIKP-PKP-Cdiff observations. Beneath the North Atlantic, the separation between the IC quasi-hemispheres appears to be located between 60A degrees W and 30A degrees W from the PKP-Bdiff observations, but it remains unresolved from the PKP-Cdiff data, due to scarce observations here.
机译:我们通过分析两对核心相位来评估地球最上层内核(IC)的平均P波速度扰动:PKIKP-PKP-Bdiff(在138.5A度-142A度的距离范围内有456次观测)和PKIKP-PKP-Cdiff(155A度-162A度的1215次观测)。前者对350-590 km深度范围内的内核速度最敏感,后者对内核边界以下0至100 km的内核速度最敏感。差分行进时间残差表现出大致“东西”的半球模式,特别是在太平洋下方。在这里,两个准半球之间的距离接近150A度的西经线(来自PKP-Bdiff观测),但可能从PKP-Cdiff转向NW-SE方向。或者,这里可能存在速度异质性,这与先前报道的PKIKP与PKPBC观测结果一致。假设IC准半球的常规定义(即QEH在0A度和180A度之间,QWH在0A度和180A度之间),准东半球表现出(+1.17 +/- 0.04)%(来自PKIKP-PKP-Bdiff)和(+0.19 +/- 0.01)%(来自PKIKP-PKP-Cdiff)的扰动。在准西半球,相应的扰动分别为(-0.06 +/- 0.06)%和(-0.19 +/- 0.02)%。印度洋地下的异常IC区在我们的PKIKP-PKP-Cdiff观测中并不明显。在北大西洋之下,IC准半球之间的距离似乎位于PKP-Bdiff观测的西经60A度和西经30A度之间,但由于这里的观测很少,PKP-Cdiff数据仍未解决。

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