小断层能否承受大应变:"岩石的脆性流动 "修订版

IF 2.9 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Earth and Space Science Pub Date : 2024-11-18 DOI:10.1029/2024EA003824
Xiaoyu Zou, Yuri Fialko
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引用次数: 0

摘要

上地壳的脆性变形被认为主要是通过断层发生的。断层长度-频率分布决定了众多小断层与少数大断层所能容纳的变形量。为了评估小断层引起的变形量,我们利用高质量的断层图分析了断层长度分布,这些断层图的空间尺度跨度很大,从实验室样本到露头再到构造域。我们发现,至少对于小于成震带厚度的断层而言,累积断层长度分布被一个负指数接近 2 的幂律很好地近似。这与地震震级-频率分布(b 值为 1 的古腾堡-里希特定律)一致。由此可见,断层是一个自相似的过程,相当一部分构造应变可以由不贯穿整个成震带的断层来承担,这与自然和实验室观测中的 "隐性应变 "推论是一致的。构造应变的持续积累最终可能导致从分布式断层网络向局部成熟断层过渡。
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Can Large Strains Be Accommodated by Small Faults: “Brittle Flow of Rocks” Revised

Brittle deformation in the upper crust is thought to occur primarily via faulting. The fault length-frequency distribution determines how much deformation is accommodated by numerous small faults versus a few large ones. To evaluate the amount of deformation due to small faults, we analyze the fault length distribution using high-quality fault maps spanning a wide range of spatial scales from a laboratory sample to an outcrop to a tectonic domain. We find that the cumulative fault length distribution is well approximated by a power law with a negative exponent close to 2. This is in agreement with the earthquake magnitude-frequency distribution (the Gutenberg-Richter law with b-value of 1), at least for faults smaller than the thickness of the seismogenic zone. It follows that faulting is a self-similar process, and a substantial fraction of tectonic strain can be accommodated by faults that don't cut through the entire seismogenic zone, consistent with inferences of “hidden strain” from natural and laboratory observations. A continued accumulation of tectonic strain may eventually result in a transition from distributed fault networks to localized mature faults.

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来源期刊
Earth and Space Science
Earth and Space Science Earth and Planetary Sciences-General Earth and Planetary Sciences
CiteScore
5.50
自引率
3.20%
发文量
285
审稿时长
19 weeks
期刊介绍: Marking AGU’s second new open access journal in the last 12 months, Earth and Space Science is the only journal that reflects the expansive range of science represented by AGU’s 62,000 members, including all of the Earth, planetary, and space sciences, and related fields in environmental science, geoengineering, space engineering, and biogeochemistry.
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