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首页> 外文期刊>Space Science Reviews >Crustal S-Wave Velocity from Apparent Incidence Angles: A Case Study in Preparation for InSight
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Crustal S-Wave Velocity from Apparent Incidence Angles: A Case Study in Preparation for InSight

机译:来自表观入射角的地壳S波速度:一种思想研究的案例研究

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Retrieval of crustal structure and thickness of Mars is among the main goals of InSight. Here we investigate which constraints on the crust at the landing site can be provided by apparent P-wave incidence angles derived from P-receiver functions. We consider receiver functions for six different Mars models, calculated from synthetic seismograms generated via Instaseis from the Green's function databases of the Marsquake Service, in detail. To allow for a larger range of crustal thicknesses and structures, we additionally analyze data from five broad-band stations across Central Europe.We find that the likely usable epicentral distance range for P-wave receiver functions on Mars lies between 35? and the core shadow, and can be extended to more than 150? by also using the PP-phase. Comparison to models for the spatial distribution of Martian seismicity indicates that sufficient seismicity should occur within the P-wave distance range around InSight within the nominal mission duration to allow for the application of our method. Apparent P-wave incidence angles are derived from the amplitudes of vertical and radial receiver functions at the P-wave onset within a range of period bands, up to 120 s. The apparent incidence angles are directly related to apparent S-wave velocities, which are inverted for the subsurface S-wave velocity structure via a grid search. The veracity of the forward calculated receiver functions and apparent S-wave velocities is ensured by benchmarking various algorithms against the Instaseis synthetics. Results indicate that apparent S-wave velocity curves provide valuable constraints on crustal thickness and structure, even without any additional constraints, and considering the location uncertainty and limited data quantity of InSight. S-wave velocities in the upper half of the crust are constrained best, but if reliable measurements at long periods are available, the curves also provide constraints down to the uppermost mantle. Besides, it is de
机译:检索出壳结构和火星厚度是洞察力的主要目标。在这里,我们调查着陆位点上的地壳上的约束可以通过来自P接收器功能的明显的p波入射角提供。我们考虑了六种不同火星模型的接收器函数,从Marsquake服务的绿色功能数据库中通过Instaseis产生的合成地震图计算。为了允许更大范围的地壳厚度和结构,我们还在中欧的五个宽带站分析数据。我们发现火星上的P波接收器功能的可能可用的震中距离范围在于35?和核心影子,可以扩展到150多个?通过使用PP相。与火星地震性空间分布的模型的比较表明,在标称任务持续时间内的洞察中,在P波距离范围内发生足够的地震性,以允许应用我们的方法。表观P波入射角来自垂直和辐射接收器的幅度,在一系列时段带内的P波开始,高达120秒。表观入射角与表观S波速度直接相关,表观S波速度通过网格搜索对地下S波速度结构反转。通过针对ISSASEIS合成的各种算法基准测试,确保了前向计算的接收器功能和表观S波速度的真实性。结果表明,即使没有任何额外的约束,表观S波速度曲线也为地壳厚度和结构提供了有价值的限制,并且考虑了位置不确定性和有限的洞察数据量。地壳的上半部分的S波速度最佳,但如果在长期的可靠测量可用,则曲线也将约束向最高的地幔提供。此外,它是de

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