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IRIS和我们星球表面
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作者 a.levander 刘希玲 《世界地震译丛》 1997年第5期6-10,共5页
地球表层的原动力产生于岩石层对使其变形的驱动力的响应。板块构造理论对海洋岩石层的运动做了很好的解释,海洋岩石层的年龄一般少于200Ma。大陆岩石层典型地记录了十亿年来的地质演化过程。即使是对现代变形,也很难估算大陆岩石层的... 地球表层的原动力产生于岩石层对使其变形的驱动力的响应。板块构造理论对海洋岩石层的运动做了很好的解释,海洋岩石层的年龄一般少于200Ma。大陆岩石层典型地记录了十亿年来的地质演化过程。即使是对现代变形,也很难估算大陆岩石层的应力平衡。假使地球应力场可以直接测量,例如,使用钻孔崩裂测量方法,也需要根据岩石层几何形态及物理状态来将这些点上的应力值外推到整个地球。实时形变的GPS测量观测的是瞬时应变场,只有用合适的本构关系才能把它和应力场联系起来。地震数据对调查我们星球表层内过去和现代运动的地下记录是很必要的。岩石层成象是不容易的,垂向和侧向上的强烈变化的范围相当于用来探测地壳结构的地震波长的范围。这些变化改变了地震波的传播途径,在地表记录的地震波场中产生复杂的图象。岩石层的结构可以描绘成一个三维非均匀波谱,这个波谱可延伸的波段很宽,且仅仅是局部稳定的,需要不同的地震探测方法来重建这种复杂的波数谱,即岩石层的结构。反射地震学为识别陆壳的细结构提供了最高分辨率手段,其分辨率在深部地壳大约为数百米,在浅部地壳可达几米。折射地震学为地壳和上地幔地震波速的变化提供了从某种程度上说更粗略一些的测量方法,其分辨率大约为数公里至数十公里,在区域地震台阵中的地方震测量可提供5~10km规模的构造信息,以及高精度的地震活动性图。在线性分布和区域性分布的便携式地震台阵中,远震信号的宽频带测量可提供地壳总体结构的信息,还可提供地幔结构的最高分辨率,通常为30km的大小。用所提供的三种方法来提高分辨率,并结合不同尺度的测量结果是地震研究的重要内容。 展开更多
关键词 IRIS 星球表面 地震观测 板块构造 地震数据
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Receiver function imaging in strongly laterally heterogeneous crust:Synthetic modeling of BOLIVAR data
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作者 a.levander 《Earthquake Science》 CSCD 2011年第1期45-54,共10页
We resolve a large (-20 km) discrepancy in Moho depth determined from PdS receiver functions (RFs) and from active source seismic profiling in the complex Caribbean-South American plate boundary zone in eastern Ve... We resolve a large (-20 km) discrepancy in Moho depth determined from PdS receiver functions (RFs) and from active source seismic profiling in the complex Caribbean-South American plate boundary zone in eastern Venezuela. As part of the BOLIVAR experiment 20 broadband stations were deployed along an active source profile to record teleseisms. Using the extremely heterogeneous crustal model obtained from active source data, we generated 2D finite-difference elastic wave synthetics and from them calculated receiver functions and CCP stacks. We compare the observations with synthetic sections that have been spatially sampled at 0.25 km to 40 km. The densely sampled synthetics show that several events in the field data that were originally interpreted as the Moho are multiple reflections within sedimentary basins. Where the Moho has the steepest dip under the plate boundary the CCP stacks fail to image the Moho well, regardless of the density of spatial sampling. A suitable spatial sampling criterion for clearly imaging the lower crust and Moho is to overlap Fresnel zones by 50% at Moho depth, which for the 1 Hz receiver functions examined here, requires an instrument spacing of 15-20 km, with the actual field data density ranging from 20 km to 100 km. 展开更多
关键词 receiver function CCP stacking finite-difference modeling BOLIVAR project Fresnel zone
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