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Testing the stress shadow hypothesis

机译:测试压力阴影假说

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A fundamental question in earthquake physics is whether aftershocks are predominantly triggered by static stress changes (permanent stress changes associated with fault displacement) or dynamic stresses (temporary stress changes associated with earthquake shaking). Both classes of models provide plausible explanations for earthquake triggering of aftershocks, but only the static stress model predicts stress shadows, or regions in which activity is decreased by a nearby earthquake. To test for whether a main shock has produced a stress shadow, we calculate time ratios, defined as the ratio of the time between the main shock and the first earthquake to follow it and the time between the last earthquake to precede the main shock and the first earthquake to follow it. A single value of the time ratio is calculated for each 10 × 10 km bin within 1.5 fault lengths of the main shock epicenter. Large values of the time ratio indicate a long wait for the first earthquake to follow the main shock and thus a potential stress shadow, whereas small values indicate the presence of aftershocks. Simulations indicate that the time ratio test should have sufficient sensitivity to detect stress shadows if they are produced in accordance with the rate and state friction model. We evaluate the 1989 M W 7.0 Loma Prieta, 1992 M W 7.3 Landers, 1994 M W 6.7 Northridge, and 1999 M W 7.1 Hector Mine main shocks. For each main shock, there is a pronounced concentration of small time ratios, indicating the presence of aftershocks, but the number of large time ratios is less than at other times in the catalog. This suggests that stress shadows are not present. By comparing our results to simulations we estimate that we can be at least 98% confident that the Loma Prieta and Landers main shocks did not produce stress shadows and 91% and 84% confident that stress shadows were not generated by the Hector Mine and Northridge main shocks, respectively. We also investigate the long hypothesized existence of a stress shadow following the 1906 San Francisco Bay area earthquake. We find that while Bay Area catalog seismicity rates are lower in the first half of the twentieth century than in the last half of the nineteenth, this seismicity contrast is also true outside of the Bay Area, in regions not expected to contain a stress shadow. This suggests that the rate change is due to a more system wide effect, such as errors in the historical catalog or the decay of aftershocks of the larger 1857 Fort Tejon earthquake.
机译:地震物理学中的一个基本问题是余震是由静态应力变化(与断层位移相关的永久应力变化)还是由动应力(与地震震荡相关的临时应力变化)引起的。两种模型都为地震余震的触发提供了合理的解释,但是只有静态应力模型才能预测应力阴影或附近地震导致活动减少的区域。为了测试主震是否产生了应力阴影,我们计算了时间比率,定义为主震与随后发生的第一次地震之间的时间与主震发生前的最后一次地震之间以及主震之间的时间之比。跟随它的第一次地震。在主震震中的1.5个断层长度内,为每个10×10 km区间计算一个时间比率值。时间比率大的值表示长时间等待第一次地震跟随主震,因此潜在的应力阴影,而小的值表示存在余震。仿真表明,如果根据速率和状态摩擦模型生成应力阴影,则时间比率测试应该具有足够的灵敏度来检测应力阴影。我们评估了1989年MW 7.0洛马普利塔(Loma Prieta),1992年MW 7.3着陆器,1994年MW 6.7诺斯里奇(Northridge)和1999 MW 7.1赫克托雷(Hector Mine)的主要冲击。对于每一次主震,都有明显的小时间比例集中,表明存在余震,但是大时间比例的数量少于目录中其他时间的数量。这表明没有压力阴影。通过将我们的结果与模拟结果进行比较,我们估计我们至少可以对Loma Prieta和Landers主震不会产生应力阴影产生98%的信心,并且可以分别对Hector Mine和Northridge主力不会产生应力阴影产生91%和84%的信心。分别震动。我们还研究了1906年旧金山湾地区地震后长期以来假设的应力阴影存在。我们发现,虽然二十世纪上半叶的湾区目录地震活动率低于十九世纪后半叶,但在湾区以外,在预计不会包含应力阴影的地区,这种地震活动性的对比也是正确的。这表明速率变化是由于更广泛的系统影响所致,例如历史目录中的错误或1857年大宗戎堡地震的余震衰减。

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