Spatio-Temporal Complexity of Aftershocks in the Apennines Controlled by Permeability Dynamics and Decarbonization

被引:14
作者
Gunatilake, Thanushika [1 ]
Miller, Stephen A. [1 ]
机构
[1] Univ Neuchatel, Ctr Hydrogeol & Geotherm CHYN, Neuchatel, Switzerland
关键词
Apennines earthquakes; Amatrice-Visso-Norcia sequence; fluid-driven aftershocks; thermal decomposition; mathematical; physical; and numerical modeling; non-linear fluid-pressure diffusion with source term; FAULT-VALVE BEHAVIOR; CO2; FLUXES; EARTHQUAKE; FLUID; SEQUENCE; RUPTURE; MODEL; SCALE;
D O I
10.1029/2022JB024154
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
In 2016, a series of large normal faulting earthquakes in the Apennines filled the seismic gap between the 1997 Colfiorito and 2009 L'Aquila earthquakes. These earthquakes, known as the Amatrice-Visso-Norcia (AVN) sequence, spawned hundreds of thousand of aftershocks in the first year, extending about 60 km along strike. The Colfiorito and L'Aquila aftershocks showed a significant high fluid-pressure component in their aftershock genesis, and here we show evidence that the AVN aftershocks also include a significant high pressure CO2 component. This CO2 is both deeply-derived, and internally generated by thermal decomposition. Using a simple model of non-linear diffusion with a source term, we compare model results with the observed cumulative number of aftershocks, and also spatial comparisons between the calculated fluid pressure and the hypocenters of about 35,000 well-located events. The good comparisons between model and observations provide evidence that the AVN sequence includes a contribution (additional fluid source) from co-seismic decarbonization. Our results suggest that internal fluid generation through devolitization or decarbonization is responsible for non-Omori type aftershock behavior such as observed for the AVN sequence and for the 2011 M-w 9.1 Tohoku (Japan) and the 2014 Iquique (Chile) M-w 8.2 megathrust subduction zone earthquakes.
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页数:11
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