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基于全球估计汇编的后滑矩缩放与变异性

Afterslip Moment Scaling and Variability From a Global Compilation of Estimates.

作者信息

Churchill R M, Werner M J, Biggs J, Fagereng Å

机构信息

School of Earth Sciences University of Bristol Bristol UK.

School of Earth and Environmental Sciences Cardiff University Cardiff UK.

出版信息

J Geophys Res Solid Earth. 2022 Apr;127(4):e2021JB023897. doi: 10.1029/2021JB023897. Epub 2022 Apr 12.

Abstract

Aseismic afterslip is postseismic fault sliding that may significantly redistribute crustal stresses and drive aftershock sequences. Afterslip is typically modeled through geodetic observations of surface deformation on a case-by-case basis, thus questions of how and why the afterslip moment varies between earthquakes remain largely unaddressed. We compile 148 afterslip studies following 53 6.0-9.1 earthquakes, and formally analyze a subset of 88 well-constrained kinematic models. Afterslip and coseismic moments scale near-linearly, with a median Spearman's rank correlation coefficient (CC) of 0.91 after bootstrapping (95% range: 0.89-0.93). We infer that afterslip area and average slip scale with coseismic moment as and , respectively. The ratio of afterslip to coseismic moment ( ) varies from <1% to >300% (interquartile range: 9%-32%). weakly correlates with (CC: -0.21, attributed to a publication bias), rupture aspect ratio (CC: -0.31), and fault slip rate (CC: 0.26, treated as a proxy for fault maturity), indicating that these factors affect afterslip. does not correlate with mainshock dip, rake, or depth. Given the power-law decay of afterslip, we expected studies that started earlier and spanned longer timescales to capture more afterslip, but does not correlate with observation start time or duration. Because estimates for a single earthquake can vary by an order of magnitude, we propose that modeling uncertainty currently presents a challenge for systematic afterslip analysis. Standardizing modeling practices may improve model comparability, and eventually allow for predictive afterslip models that account for mainshock and fault zone factors to be incorporated into aftershock hazard models.

摘要

无震余滑是震后断层滑动,可能会显著重新分布地壳应力并引发余震序列。余滑通常是通过逐案对地表变形进行大地测量观测来建模的,因此关于余滑矩在不同地震之间如何以及为何变化的问题在很大程度上仍未得到解决。我们汇总了53次6.0 - 9.1级地震后的148项余滑研究,并正式分析了88个约束良好的运动学模型的子集。余滑矩和同震矩近线性缩放,自展后斯皮尔曼等级相关系数(CC)的中位数为0.91(95%范围:0.89 - 0.93)。我们推断余滑面积和平均滑动分别与同震矩按 和 缩放。余滑与同震矩的比值( )从<1%到>300%不等(四分位间距:9% - 32%)。 与 (CC: - 0.21,归因于发表偏倚)、破裂长宽比(CC: - 0.31)和断层滑动速率(CC:0.26,视为断层成熟度的代理指标)弱相关,表明这些因素会影响余滑。 与主震倾角、滑动角或深度无关。鉴于余滑的幂律衰减,我们预计开始时间较早且跨越较长时间尺度的研究会捕获更多余滑,但 与观测开始时间或持续时间无关。由于单次地震的 估计值可能相差一个数量级,我们提出建模不确定性目前是系统余滑分析面临的一个挑战。规范建模方法可能会提高模型的可比性,并最终使考虑主震和断层带因素的预测性余滑模型能够纳入余震灾害模型。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ab6e/9287082/7b53888e149d/JGRB-127-0-g010.jpg

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