Abstract
Characterising the state of stress in the brittle uppercrust is essential in mechanics of faulting, industrial production processes, and operational earthquake forecasting. Nevertheless, unresolved questions concern the variation of porefluid with depth and the absolute strength on tectonically active faults. Here we show that, along the San Andreas fault system, the timedelay before the onset of the powerlaw aftershock decay rate (the cvalue) varies by three orders of magnitude in the first 20 km below the surface. Despite the influence of the lithostatic stress, there is no continuous change in cvalue with depth. Instead, two decay phases are separated by an abrupt increase at an intermediate depth range of 2–5 km. This transitional regime is the only one observed in fluidinjectioninduced seismic areas. This provides strong evidence for the role of fluid and a porosity reduction mechanism at depth of few kilometres in active fault zones. Aftershock statistics can then be used to predict changes in differential shear stress with depth until the brittleductile transition is reached.
Introduction
Despite an increasing number of observations along the San Andreas fault system, no consensus has been reached about the absolute strength of the major strikeslip faults that accommodate the rightlateral motion between the Pacific and North American plates^{1,2,3,4,5,6,7}. The absence of heat flow anomaly near the major fault segments^{4} as well as the apparent high angle between these fault planes and the direction of the maximum horizontal compressive stress^{1} suggest an extremely weak fault in term of friction coefficient^{8}. Other arguments related to stress rotation in transpressional plate boundaries support a strongfault hypothesis^{6}. In all debates, the role of fluids has to be considered because pore pressure may linearly compensate for the overburden pressure at depth^{5,9}. Under such condition, the frictional strength of faults decreases significantly as the pore pressure increases in excess to hydrostatic^{10}. Hence, changes in pore pressure have been proposed as a generic mechanism for seismicity and aftershock sequences^{11,12,13}. This mechanism has been extensively studied in mining or fluid injection sites where fluid pressure and stress diffusion may trigger seismic events or considerably change the earthquake rate^{14,15,16,17}. However, there is still no wellestablished relation between earthquake statistics and pore pressure along active tectonic faults.
Direct measurements of the stress magnitude in the brittle uppercrust relies on drilling methods using hydraulic fractures and wellbore breakouts^{1,18}. Due to the needs for large and homogeneous samples to examine the level of stress along active fault zones, indirect measurements are still required and earthquakes continue to provide the most informative data for comparative analysis^{19,20,21}. Stress directions are generally derived from inversion of focal mechanisms^{22,23}. Independently, earthquake catalogues are increasingly used to infer changes in stress intensity from deviations of wellknown distributions in statistical seismology^{24}. The two main parameters under investigation are the slope of the earthquake size distribution, the bvalue^{25}, and the time delay before the onset of the powerlaw aftershock decay rate, the cvalue^{26}. As the time for nucleation and growth of brittle cracks is likely to decrease with the level of stress^{27}, it was proposed that b and cvalues reflect the same failure mechanisms within the process zone and the aftershock area during and after the dynamic rupture, respectively. Then, as shown from observations, they both exhibit the same negative dependence on stress^{24,25}.
Here, we concentrate on aftershock sequences along the San Andreas fault system to evaluate how the cvalue varies with depth. We show that a sharp increase in cvalue at intermediate depth of 2–5 km separates two decay phases with different slopes. These three different phases of the cvalue vertical profile are consistent with variations in stress predicted by the Anderson’s faulting theory and the Coulomb faulting theory considering a porosity reduction mechanism at intermediate depth. We conclude that such variations of stress magnitude can naturally explain changes in earthquake statistics with depth, as well as the apparent weakness of faults along major strikeslip faults in California.
Results
Vertical cvalue profiles in California
We examine aftershock sequences along the San Andreas fault system using the hypocenter information of the modern waveform relocated catalogues for southern and northern California from 1984 to 2016^{28,29,30}. To identify mainshocks, we deselect earthquakes of magnitude smaller than M which are within a 0.02 × 10^{0.5M} km radius circle during the first 0.04 × 10^{0.55M} days after a magnitude M event^{31}. Keeping the same spatial scaling, earthquakes that precede larger events by less than 24 h are classified as potential foreschocks. All the remaining events are mainshocks. Their respective aftershocks are selected in the time interval [t _{start}, t _{stop}] after the mainshock time using again the same spatial scaling. For t _{start} = 10 s, t _{stop} = 1 day and M ≥ 2.5, we obtain nonoverlapping aftershock sequences from which we can analyse the early aftershock decay rate.
Another critical issue of our declustering method is that the selected earthquakes are classified in ranges of magnitude. Here, we focus only on 2.5 < M ^{M} < 3.5 mainshocks and 1.8 < M ^{A} < 2.8 aftershocks. By analysing only large aftershocks of small mainshocks, we do not only reduce artefacts related to catalogue completeness over short time, we also study narrow ranges of magnitude over which c keeps a relatively large and constant value^{32,33}. To reduce the impact of faulting style on cvalues, we select only mainshocks along a set of welldefined subvertical strikeslip faults in narrow bands of 15 km wide down to focal depths of 20 km. Ultimately, we analyse 3000 aftershock sequences comprising 4839 events within the first day after the mainshock (1668 and 3295 in southern California, 1332 and 1544 in northern California). Then, we stack aftershocks according to the mainshock time to compensate for the small number number of events in each sequence.
We use uniform priors in a Bayesian estimation of the parameters of the Modified Omori Law,
to characterise the exponent p of the powerlaw aftershock decay rate and the duration c of the early stage of aftershock activity that does not fit with this powerlaw regime^{34}. From the entire stacked sequence, Fig. 1 shows the Bayesian posterior densities of {c, p} for shallow (4–6 km) and deep (9–13 km) aftershocks. These two distributions do not overlap below their 99% interior range, so that there are statistically significant differences between shallow and deep aftershock sequences along strikeslip faults in California. The incompatibility between these two distributions resides more in the cvalue than in the pvalue as indicated by the marginal posterior distributions of these two parameters (Fig. 1). This suggests that the time delay c is more sensitive to depth than the powerlaw exponent p (see “Methods” section). Hence, we document only variations in cvalue estimating the parameters of the original Omori formula Λ(t) = K/(c + t). Thus, we reduce the uncertainty imposed by the positive dependence on the estimation of both {c, p}values^{34}. In addition, we can also recover the variation of cvalue using the \(\left\langle {{t_g}} \right\rangle \)value, the geometric mean of aftershock times over the same time period [t _{start}, t _{stop}] (see “Methods” section). This nonparametric estimator of the time delay before the onset of the powerlaw aftershock decay rate is free from uncertainties related to the fitting procedure and do not rely on the validity of the Modified Omori Law^{35}.
For each strikeslip fault under investigation, we isolate the corresponding stack of aftershocks and select them according to depth using a sliding window with a thickness of 3 km and a step of 0.3 km. Figure 2 shows the evolution of cvalues with respect to depth for all these faults. Despite some variations related to the spatial distribution of seismicity in these specific areas and overlapping error bounds, a similar behaviour may be observed across the entire California: a sharp increase in cvalue at shallow depth (≤5 km) is followed by a continuous decrease to depth of about 15 km. As a result, the cvalue may drop by more than two orders of magnitude from 15 mn at depth of 5 km to 20 s in the neighbourhood of the brittleductile transition zone. These estimates are obtained from independent sets of events, mainly in southern California where a larger number events occur over a wider depth range (e.g., San Andreas and San Jacinto faults). In all places, the continuous change in cvalue is due to the moving step of the overlapping slidingwindow for event selection, which gradually replaces a small proportion of aftershocks in the stacks. Finally, the dependence of the cvalue on depth is tested by checking that similar signals can be recovered using the \(\left\langle {{t_g}} \right\rangle \)value and a different declustering procedure^{36,37,38} (see “Methods” section).
To explain these vertical cvalue profiles, the stress magnitude at depth may be directly estimated from the Anderson faulting theory and limited by Coulomb faulting theory, which gives the maximum values of the differential shear stress before failure (see “Methods” section). Considering a constant friction coefficient^{8}, the increase of the lithostatic stress with depth results in a linear increase of the minimum differential stress to initiate slip along preexisting faults. Then, the systematic decrease in cvalue in the depth interval from 5 to 15 km agrees with previous studies concluding that the time delay before the onset of the aftershock decay rate is negatively correlated to the differential shear stress^{24,32,39,40}. On the opposite, the abrupt increase in cvalue occurring in the shallow part of the crust (<5 km) cannot be explained by the linear increase of the lithostatic stress. To investigate this anomalous behaviour, we analyse the triggered seismicity in the neighbourhood of two industrial injection sites^{41,42}, the Geyser and the Salton Sea geothermal plants. Using all earthquakes in two circles of 10 km radius centred at (38°06″N, 122°48″W) and at (33°12″N, 115°36″W), we apply the same procedure as along strikeslip faults to identify mainshockaftershocks sequences. Figure 3 shows the evolution of the cvalue with respect to depth for these two geothermal areas. In Geysers, a zone where all the seismicity is triggered by fluid injection, there is no earthquake below 5 km. In Salton Sea, where natural and fluidinduced earthquakes coexist, seismic events are observed to depth of 8 km. Despite all the differences between these two sites, they both exhibit the same cvalue behaviour with respect to depth: a drastic increase of more than three orders of magnitudes from depth of 2 km to depth of 6 km. Such a behaviour can be directly compared to cvalue variations at shallow depth along strikeslip faults, thereby shedding light on the role of fluid in these active fault zones.
In geothermal areas, the observed seismicity and local stresses are directly correlated to fluidinjection operations. The triggered seismic activity may then be associated with a relaxation process of stress and pore pressure in both space and time. Such a mechanism may naturally explain the increase in cvalue with depth, i.e., with the distance from the injection source. Along strikeslip faults, we infer that a porosity reduction mechanism at depth of few kilometres could play the same role and strongly reduce the strength of preexisting fractures.
In order to account for a porosity reduction mechanism in the Coulomb faulting theory, we propose a model for the evolution of the pore pressure with depth (Fig. 4a, see also “Methods” section). Since we concentrate on statistical properties that are averaged over space and time, we consider that pore pressure does not operate a sharp jump from its hydrostatic to its nearlithostatic regimes. Instead, below a threshold depth z _{c}, we assume that the transition between these two regimes takes the form of an exponential relaxation with a characteristic thickness L (Fig. 4a). Combining the fault strength derived from this pore pressure profile with a creep rheology usually used to describe the brittleductile transition at larger depth (see “Methods” section), Fig. 4b shows the strength envelop for a friction coefficient μ = 0.75. The variation of cvalue is superimposed on this strength envelop using a different axis on the same graph. The comparison between these two signals reveal striking similarities at all depths. At intermediate depth between 2 and 5 km (i.e., z _{c} = 2 km and L = 1 km), the transition from hydrostatic to nearlithostatic porepressure conditions gives the depthrange within which the cvalue increases. Above and below this transition layer, the rapid and slow increases in cvalue are governed by the increase in lithostatic stress under hydrostatic and nearlithostatic porepressure conditions, respectively. Finally, for depth larger than 15 km, intercrystalline plasticity is thermally activated, creep dominates and the differential shear stress collapses. A transition which is also captured by the cvalue.
Discussion
The depthdependent behaviour of the cvalue is not a consequence of background contamination or an artefact related to the working assumption of p = 1. It can be independently recovered for southern and northern California estimating simultaneously the background seismicity and both the c and pvalues (see “Methods” section). However, local properties along faults in California are likely to differ and, because we rely on a limited amount of data, they cannot be individually inferred from aftershocks. This is why the overall effect of the confining stress and porepressure should be averaged at the length scale of California considering only events along major strikeslip faults.
The vertical cvalue profiles presented in Figs. 2 and 4 illustrate how the differential stress control the duration of the preliminary phase of aftershock sequences at all depths across the brittle uppercrust. Similar results have been obtained for the slope b of the earthquake size distribution^{43}. A monotonic decrease in bvalue between 5 and 15 km as well as a rapid increase below the brittleductile transition may be directly linked with similar behaviours of the cvalue over the same depth intervals. In addition, an increase in bvalue with respect to depth has also been documented at shallow depth (<5 km), but not interpreted. This symptomatic behaviour can reflect the porosity reduction mechanism revealed by aftershocks (Fig. 4). In this case, the magnitude of stress usually proposed from the slope b of earthquake size distribution^{44} may be overestimated and warrant further investigation.
Using small magnitude events occurring along strikeslip faults in California, aftershock statistics show that the characterisation of the state of stress in the brittlecrust should account for near lithostatic porepressure conditions. These conditions appear to be associated with a porereduction mechanism as a result of a loss of structural connectivity and fluid trapping within the fracture networks of active fault zones. As predicted by theory and observed from aftershocks, this most likely occurs in the vicinity of a percolation threshold at intermediate depth between 2 and 5 km. Within this transition layer, both the fracture strength and the frictional strength decrease significantly to levels which could explain the apparent weakness of faults at this depth and deeper, where most of the seismic energy is released, in the depth range between 5 and 15 km. Such a control of porepressure on the aftershock decay rate support the increasing body of evidence highlighting the role of fluids along the San Andreas fault system, a necessary ingredient for the weak fault model. Moreover, the present study shows that aftershocks may provide indirect estimates of the magnitude of stress through the variation of wellestablished statistical parameters. This information could now be used to develop new quantitative methods not only in the physics of faulting and seismic hazard studies but also in industrial settings where deep injection of fluids are known to produce earthquakes.
Methods
Frictional rheology
The Mohr–Coulomb theory proposes that shear failure in a homogeneous medium subject to a uniform triaxial stress {σ _{1}, σ _{2}, σ _{3}} should occur on optimally oriented planes. These planes are parallel to the intermediate shear stress σ _{2} and form an angle Θ with σ _{1}, the maximum compressive stress. Then, the condition for faulting is governed by:
where μ is a coefficient of static friction, and σ _{n} and τ are the normal stress and the shear stress resolved on the fault surface. This condition may be rewritten in terms of the principal stresses in order to determine with respect to μ the angle Θ and the differential shear stress (σ _{1} − σ _{3}) at which faulting may occur^{45}. In this context, the orientation of the principal shear stresses not only determines the faulting mechanism but also the amplitude of the differential shear stress.
The effective overburden stress at a depth z in the crust is:
where ρ _{r} is the crustal density, g the acceleration due to gravity, and 0 ≤ λ ≤ 1 the pore fluid factor. In practice, we have
where P is the porefluid pressure and P _{lith} = ρ _{r} gz the lithostatic pressure. Following the Anderson’s theory of faulting, the minimum differential stress to initiate slip at a given depth and fluid pressure is:
where q = 0 for thrust faults,
for strikeslip faults, q = 1 for normal faults, and
Pore pressure depth profile
To explain the vertical cvalue profiles observed along strikeslip faults in California (Figs. 2, 4), we consider a change in pore pressure regime with respect to depth. In practice, we assume that the pore pressure P operates a transition from hydrostatic to nearly lithostatic as depth exceeds a threshold value z _{c}. Thus, below this critical depth, the reduction of porosity and permeability generate isolated pockets of excess pore pressure. As these pockets increase in number and size according to depth, there is a continuous loss of pore connectivity, which could be associated with a rapid increase in pore pressure. Ultimately, it should be associated with a percolation threshold. Nevertheless, to account for spatial and temporal heterogeneities at the scales of the stacks of aftershocks under examination in this study, we consider an exponential relaxation of the pore fluid factor of the form:
where ρ _{w} is the density of water, L a characteristic length for a complete loss of pore connectivity, and ε the ratio of pore pressure to lithostatic stress at great depth (i.e., \(z \gg {z_{\rm{c}}} + L\)). All the parameter values for this pore pressure depth profile are given in Table 1 (see also the inset in Fig. 4).
Creep rheology
Intercrystalline plasticity is a thermally activated process^{46}, which is responsible for the brittleductile transition at depth. For a given strain rate \(\dot \varepsilon \), the differential shear stress of a steadystate flow of rocks by intercrystalline processes obeys a relationship of the form:
where E is an activation energy, n the stress exponent, R the gas constant, T the absolute temperature, and A a constant^{47}.
Strength envelope
In order to determine strength envelopes, the strength at any given depth is the lower of the brittle and ductile differential shear stress (see Eqs. (5) and (9), respectively). For the strength envelope in Fig. 4, we consider strikeslip faulting, σ _{2} = σ _{v} (Supplementary Fig. 1) and
All the other parameter values of Eqs. (5) and (9) are shown in Table 1.
Spacetime parameterisation of the declustering procedure
Studying more than 30 years of seismicity, the quality of the catalogues may have changed for the magnitude range under investigation. We compare two time periods, 1984–2000 and 2001–2016, considering together all the aftershocks selected along major subvertical strikeslip faults in California (Fig. 2). The vertical cvalue profiles are similar for the two time periods (Supplementary Fig. 2), indicating that there is no influence of catalogue completeness on the depthdependent behaviour.
Along major strikeslip faults, the majority of slip is confined in narrow layers^{48} within a wider zone of damage, the socalled fault zone. To estimate how the vertical cvalue profile varies across fault zones, we vary the width (Supplementary Fig. 3a) and the position (Supplementary Fig. 3b) of the layer in which we select mainshocks and aftershocks. The depth dependence of the cvalue is stable up to a distance of 15 km from the faults. At greater distances, cvalues are larger and show no systematic variation with respect to depth. A tendency of smaller cvalues at shorter distances from faults is observed in most depth ranges.
The vertical cvalue profile is computed from the average depth of aftershocks in each depth range. Similar results are obtained using the average depth of mainshocks (Supplementary Fig. 4), except in the neighbourhood of the brittlecreep transition below 13 km, where triggered events are likely to represent a higher proportion of seismicity than in the brittle upper part of the crust^{49}.
Both the spatial and temporal windows of the declustering procedure scale with the magnitude M of the mainshocks: R = 0.02 × 10^{0.5M} is the radius of influence expressed in kilometres; T = 0.04 × 10^{0.55M} is the time of influence expressed in days. Leaving the scaling exponents unchanged, the same vertical cvalue profiles are obtained when increasing or decreasing T and Rvalues by a factor 2 (Supplementary Fig. 5).
Influence of the magnitude ranges on the cvalue depth profile
All cvalues are computed for \(M_{{\rm{min}}}^{\rm{A}} \le {M^{\rm{A}}} \le M_{{\rm{max}}}^{\rm{A}}\) aftershocks of \(M_{{\rm{min}}}^{\rm{M}} \le {M^{\rm{M}}} \le M_{{\rm{max}}}^{\rm{M}}\) mainshocks within the time interval [t _{start}, t _{stop}]. These six parameters {\(M_{{\rm{min}}}^{\rm{A}}\), \(M_{{\rm{max}}}^{\rm{A}}\), \(M_{{\rm{min}}}^{\rm{M}}\), \(M_{{\rm{max}}}^{\rm{M}}\), t _{start}, t _{stop}} have a regular effect on the cvalue, which is negligible compared to the influence of depth through the brittle crust. An increase of the \(M_{\rm{A}}^{{\rm{min}}}\)value or a higher range \(\left[ {M_{\rm{A}}^{{\rm{min}}},M_{\rm{A}}^{{\rm{max}}}} \right]\) of aftershock magnitude lead to smaller cvalues almost at all depths (Supplementary Fig. 6a, c). Meanwhile, a change in \(M_{\rm{A}}^{{\rm{max}}}\)value for \(M_{\rm{A}}^{{\rm{min}}} = 1.8\) has no influence on cvalues (Supplementary Fig. 6b). An increase of \(M_{\rm{M}}^{{\rm{min}}}\), \(M_{\rm{M}}^{{\rm{max}}}\) or a higher range \(\left[ {M_{\rm{M}}^{{\rm{min}}},{\kern 1pt} M_{\rm{M}}^{{\rm{max}}}} \right]\) of mainshock magnitude lead to higher cvalues, especially close to the depth of the brittleductile transition (Supplementary Fig. 6d–f). Finally, cvalues show no dependence on the time window [t _{start}, t _{stop}] (Supplementary Fig. 6g, h). These variations in cvalue with the difference between mainshock and aftershock magnitudes are consistent with recent findings from Davidsen and Baiesi^{50}.
The declustering method
Other declustering methods should also lead to same vertical cvalue profiles. Here, we test an alternative approach dedicated to the identification of earthquake clusters using nearest neighbour distance in timespacemagnitude domains^{36,37,38}.
For each pair of earthquakes {i, j}, we compute the proximity function^{51},
where t _{ ij } = t _{ j } − t _{ i } is the event intercurrence time, r _{ ij } the spatial distance between the epicentres, m _{ i } the magnitude of event i, d _{f} the fractal dimension of the epicentres, and b the slope of the earthquakesize distribution. Then, we construct families of nearest neighbours using a threshold ν _{0} for the proximity function^{36,38}. The ν _{0}value determines the maximum timespacemagnitude distance between parents and offsprings. Each offspring in a family has only one parent, the closest event using the proximity function. Each parent may have several offsprings. A family may consist of several generations of offsprings. In order to identify direct aftershocks, we select only the firstgeneration offsprings of the largest magnitude event in each family.
Using the proximity function and firstgeneration offspring events, Supplementary Figs. 7 and 8 show the same behaviours as in Figs. 2a and 4, respectively. The parameterisation {ν _{0}, b, d _{f}} of this new declustering method has no effect on these results for ν _{0} ∈ [10^{−7}; 10^{−3}], b ∈ [0.8; 1.2], and d _{f} ∈ [1.3; 2] (Supplementary Fig. 9a–c). The similarities between the results obtained by the two declustering methods indicate that changes in cvalues are not due to artefacts arising from a specific method. In addition, using all generation offsprings, the dependence on depth of the cvalue is not as clear as the one observed using only firstgeneration aftershocks (Supplementary Fig. 9d). This confirms the importance of the stress perturbation induced by the mainshock and also suggests that the current parameterisation of our windowbased declustering method is likely to isolate aftershock sequences mainly composed of direct aftershocks, i.e., firstgeneration offsprings (see the {\(M_{{\rm{min}}}^{\rm{A}}\), \(M_{{\rm{max}}}^{\rm{A}}\), \(M_{{\rm{min}}}^{\rm{M}}\), \(M_{{\rm{max}}}^{\rm{M}}\), t _{stop}}values in Supplementary Fig. 6).
Background activity and {c, p}values
The simultaneous estimation of both c and pvalues gives the same dependence on depth of the cvalue as that observed for p = 1 (Supplementary Fig. 10). Despite more dispersion of these estimates and a signal with lower amplitude when the pvalue is not fixed, the same transient increase in cvalue is observed at intermediate depth between 2 and 5 km. The continuous cvalue decreases below 6 km exhibit also the same slope in all cases. The pvalue is quite constant at all depths (p ≲ 1) with variations that show no positive correlation with those of the cvalue. Then, except for shallow events (<4 km) in southern California, the posterior dependence between c and p has a smaller impact than depth on both parameter estimates.
Except for the first two kilometres, the level of seismic noise in the aftershock sequences is quite uniform at all depths and never exceed 20% (red dots in Supplementary Fig. 10). Over the first day before and after the mainshocks, these levels of noise in the aftershock sequences correspond to seismic rates which are on the same order of magnitude as the rates of foreshock occurrence (dark green dots in Supplementary Fig. 10).
Using our declustering method, many mainshocks are not associated with aftershocks, especially at shallow depth (see pink and light green dots in Supplementary Fig. 10). Considering together all mainshockaftershocks sequences, our selection procedure agrees with the Bath law that states that a mainshock of M = 3 (the mean value of the mainshock magnitude range) should have on average one aftershock with M ≥ 1.8.
Northern and southern California
The depthdependent behaviour of aftershock statistics are similar for the entire California and separately for northern and southern California (Supplementary Fig. 10). In all areas, a rapid increase in cvalue at intermediate depth (≤5 km) is followed by a continuous decrease to depth of about 15 km. The larger number of events in southern California allows to investigate a wider range of depth and reduce uncertainties on both c and pvalues estimates. In southern California, the cvalue varies over a range which is an order of magnitude larger than that in northern California. Hence, the Bayesian posterior densities of {c, p} in southern California show a more distinct separation between shallow and deep aftershocks than in northern California (Supplementary Fig. 11). In both areas, most of the differences are associated with changes in cvalues despite the posterior dependency between the parameters c and p of the Modified Omori Law^{34}.
A nonparametric estimator of the cvalue
Considering a single aftershock sequence, we define \(\left\langle {{t_g}} \right\rangle \) as the geometric mean of elapsed times from mainshocks to aftershocks within a fixed time window [t _{start}, t _{stop}]:
where t _{i}, i ∈ [1, 2, …, n], is the time between the ith aftershock in [t _{start}, t _{stop}] and the mainshock. If the aftershock decay rate follows the Omori–Utsu law, λ(t) = K/(t + c), Shebalin et al.^{35} have shown that \(\left\langle {{t_g}} \right\rangle \) is an implicit function of c, t _{start}, and t _{stop} (and not K). Accordingly, the arithmetic mean of the logarithms of the elapsed times from the mainshock to aftershocks,
may be used as an estimator for the logarithm of the cvalue. Because it can be easily compute from aftershock times without a fitting procedure, the \(\left\langle {{t_g}} \right\rangle \)value is first used to identify systematic variations of the characteristic time before the onset of the powerlaw aftershock decay rate^{52}. Then, the cvalue may be estimated using the solution of an explicit equation (Eq. (9) in Shebalin et al.^{35}). This property is valid for a stack of aftershock sequences with a constant cvalue. For stacks of aftershock sequences with different cvalues, the distribution will not exactly follow the Omori–Utsu law, but averaging on the logarithm of times still make sense, given an estimate of the corresponding mean value.
Similar dependences on depth are observed using the Bayesian estimates of the cvalue or the geometric mean \(\left\langle {{t_g}} \right\rangle \) of elapsed times from mainshocks to aftershocks (Supplementary Figs. 12–14). The largest deviations are in cases of small number of aftershocks in the analysis (large error bars). However, the difference between the two procedures may be quite regular in specific seismic zones. For example, the difference is near constant at all depths along the Imperial and Laguna Salada faults. In Geysers and Salton Sea waterinjection sites the difference has an opposite sign.
Data availability
The data that support the findings of this study are available from the corresponding author upon reasonable request. The python package to perform Bayesian analysis of the Modified Omori Law can be downloaded from http://www.ipgp.fr/~narteau/.
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Acknowledgements
We acknowledge financial support of C.N. from the UnivEarthS LabEx programme of Sorbonne Paris Cité (ANR10LABX0023 and ANR11IDEX000502), the French National Research Agency (ANR12BS0500103/EXODUNES), and of P.S. from the Russian Science Foundation, Project 161700093.
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P.S. and C.N. designed the study and wrote the manuscript together. P.S. performed the data analysis. C.N. worked on the interpretation of results.
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Shebalin, P., Narteau, C. Depth dependent stress revealed by aftershocks. Nat Commun 8, 1317 (2017). https://doi.org/10.1038/s4146701701446y
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DOI: https://doi.org/10.1038/s4146701701446y
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