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首页> 外文期刊>Bulletin of the Seismological Society of America >Uncertainty in Earthquake Source Imaging Due to Variations in Source Time Function and Earth Structure
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Uncertainty in Earthquake Source Imaging Due to Variations in Source Time Function and Earth Structure

机译:由于震源时间函数和地球结构的变化,震源成像的不确定性

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One way to improve the accuracy and reliability of kinematic earthquake source imaging is to investigate the origin of uncertainty and to minimize their effects. The difficulties in kinematic source inversion arise from the nonlinearity of the problem, nonunique choices in the parameterization, and observational errors. We analyze particularly the uncertainty related to the choice of the source time function (STF) and the variability in Earth structure. We consider a synthetic data set generated from a spontaneous dynamic rupture calculation. Using Bayesian inference, we map the solution space of peak slip rate, rupture time, and rise time to characterize the kinematic rupture in terms of posterior density functions. Our test to investigate the effect of the choice of STF reveals that all three tested STFs (isosceles triangle, regularized Yoffe with acceleration time of 0.1 and 0.3 s) retrieve the patch of high slip and slip rate around the hypocenter. However, the use of an isosceles triangle as STF artificially accelerates the rupture to propagate faster than the target solution. It additionally generates an artificial linear correlation between rupture onset time and rise time. These appear to compensate for the dynamic source effects that are not included in the symmetric triangular STF. The exact rise time for the tested STFs is difficult to resolve due to the small amount of radiated seismic moment in the tail of STF. To highlight the effect of Earth structure variability, we perform inversions including the uncertainty in the wavespeed only, and variability in both wavespeed and layer depth. We find that little difference is noticeable between the resulting rupture model uncertainties from these two parameterizations. Both significantly broaden the posterior densities and cause faster rupture propagation particularly near the hypocenter due to the major velocity change at the depth where the fault is located.
机译:提高运动地震震源成像精度和可靠性的一种方法是研究不确定性的成因,并将其影响降至最低。运动源反演的困难源于问题的非线性,参数化中的非唯一选择以及观测误差。我们特别分析与源时间函数(STF)的选择和地球结构变化有关的不确定性。我们考虑由自发动态断裂计算产生的综合数据集。使用贝叶斯推论,我们绘制了峰滑移率,破裂时间和上升时间的解空间,以根据后验密度函数表征运动破裂。我们对选择STF的效果进行调查的测试表明,所有三个测试过的STF(等腰三角形,加速时间分别为0.1和0.3 s的正则Yoffe)恢复了高滑移率和低震源附近的滑移率。但是,使用等腰三角形作为STF会比目标溶液人工加速破裂传播的速度。另外,它在破裂开始时间和上升时间之间产生了人为的线性关系。这些似乎可以补偿对称三角STF中未包含的动态源效应。由于STF尾部的辐射地震矩较小,因此难以确定测试STF的确切上升时间。为了突出地球结构变化的影响,我们进行了反演,包括仅波速的不确定性以及波速和层深度的变化。我们发现这两个参数化所导致的破裂模型不确定性之间没有什么明显的区别。由于断层所在深度处的主要速度变化较大,两者都显着拓宽了后方的密度,并引起更快的破裂传播,特别是在震源附近。

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