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Possible correlation between annual gravity change and shallow background seismicity rate at subduction zone by surface load

Abstract

The Gravity Recovery and Climate Experiment (GRACE) has monitored global gravity changes since 2002. Gravity changes are considered to represent hydrological water mass movements around the surface of the globe, although fault slip of a large earthquake also causes perturbation of gravity. Since surface water movements are expected to affect earthquake occurrences via elastic surface load or pore-fluid pressure increase, correlation between gravity changes and occurrences of small (not large) earthquakes may reflect the effects of surface water movements. In the present study, we focus on earthquakes smaller than magnitude 7.5 and examine the relation between annual gravity changes and earthquake occurrences at worldwide subduction zones. First, we extract amplitudes of annual gravity changes from GRACE data for land. Next, we estimate background seismicity rates in the epidemic-type aftershock sequence model from shallow seismicity data having magnitudes of over 4.5. Then, we perform correlation analysis of the amplitudes of the annual gravity changes and the shallow background seismicity rates, excluding source areas of large earthquakes, and find moderate positive correlation. It implies that annual water movements can activate shallow earthquakes, although the surface load elastostatic stress changes are on the order of or below 1 kPa, as small as a regional case in a previous study. We speculate that periodic stress perturbation is amplified through nonlinear responses of frictional faults.

Introduction

Fault slips of earthquakes can perturb the Earth’s gravity field (Imanishi et al. 2004; Han et al. 2006), as formulated in elastomechanics (Okubo 1991; Sun and Okubo 1998). Larger earthquakes cause greater perturbation of gravity. Only large earthquakes remain the gravity signals, because of limitation in accuracy of gravity measurement.

By contrast, since gravity changes mainly reflect annually varying shallow water storage as discussed in Hydrology (e.g., Wahr et al. 2004), we expect another relation between earthquakes and gravity changes: some shallow earthquakes may be triggered by water movement around the surface (e.g., Bettinelli et al. 2008; Johnson et al. 2017). In this relation, not only large earthquakes but also small earthquakes should be involved. The physical origins of the earthquake triggering due to water movement around the surface are effects of pore-fluid pressure increase (e.g., Talwani et al. 2007) or elastic surface load (e.g., Heki 2003) on faults.

Nowadays, the Gravity Recovery and Climate Experiment (GRACE) satellites have allowed us to monitor large-scale mass movements. The GRACE satellites investigate 100- to 1000-km-scale gravity changes with an interval of approximately 1 month and can detect great perturbations of gravity due to large (> Mw 8.2) earthquakes (Han et al. 2006; Heki and Matsuo 2010; Han et al. 2013; Tanaka et al. 2015b). However, the relation between gravity changes and small earthquakes that may represent the earthquake triggering mechanisms is not well investigated.

Thus, we examine whether the GRACE gravity changes correlate with occurrences of (small) earthquakes on a global scale. We especially focus on plate subduction zones where earthquakes concentrate.

Materials and methods

Gravity data

We use GRACE level-3 gravity data for land, represented by equivalent water thickness (units: cm), from April 2002 to July 2016, provided by the Physical Oceanography, Distributed Active Archive Center at JPL (Swenson and Wahr 2006; Landerer and Swenson 2012; Swenson 2012). These data were scaled with a worldwide hydrology model in the Global Land Data Assimilation System (Rodell et al. 2004). In particular, we use the GRACE gravity data (analyzed by UTCSR) multiplied by a scaling factor at each spatial grid. Originally, the spatial grid is 1 degree square in latitude and longitude, and a 300-km-wide Gaussian filter to reduce spatial noise is applied. Hence, we spatially average the data every 10 degrees of latitude/longitude only for the grids with finite values (and excluding cases of very few grids), although an actual scale of surface water load may be smaller especially in islands area. The time-series data represent anomalies relative to the 2004.0–2009.999 time–mean baseline. The sampling interval is approximately 1 month. For deficient time-series data, we linearly interpolate the data from the last and the next data. About 10% of the time-series data (18/172) are interpolated.

The temporal gravity change (∆g) with time t (month) at each spatial grid is modeled as

$$\Delta g(t) = A + Bt + C\cos \left( {2\pi t/12} \right) + D\sin \left( {2\pi t/12} \right)$$
(1)

where the first term on the right-hand side (A) represents an offset, the second term (Bt) represents a linear trend, and the residual terms represent annual change. Using observation Eq. (1) for the gravity change, we estimate coefficients A, B, C, and D by linear regression using QR decomposition. In the following section, we use the amplitude of the annual gravity change \(\sqrt {C^{2} + D^{2} }\). Further, we tried adding terms of semi-annual change to Eq. (1), but the amplitude of the annual change did not almost change.

Earthquake data

In order to evaluate the occurrence of earthquake, we use the ANSS Comprehensive Earthquake Catalogue data from the United States Geological Survey (USGS). We consider only shallow earthquakes at subduction zones, the focal depths of which are shallower than 30 km. Since earthquake occurrences consist of aftershocks (Omori 1894) and other types of background seismicity, we extract the background seismicity rate, μ, using the epidemic-type aftershock sequence (ETAS) model (Ogata 1988).

In the ETAS model, the seismicity rate λ(t) at time t is the sum of the background seismicity rate μ and the prior aftershock sequences and is given by

$$\lambda (t) = \mu + \mathop \sum \limits_{{t_{i} \le t}} \frac{{Ke^{{\alpha \left( {M_{i} - M_{c} } \right)}} }}{{(t - t_{i} + c)^{p} }}$$
(2)

where M i is the magnitude of the ith earthquake during the observation period, M c is the minimum earthquake magnitude, and the other parameters (K, c, α, and p) are constants.

In order to estimate the five ETAS parameters in logarithmic form (log μ, log K, log c, log α, and log p), we adopt two optimization methods for comparison: a limited-memory modification of the quasi-Newton method with box constraints (Byrd et al. 1995) and the differential evolution method (Storn and Price 1997) that is a kind of evolutionary computation to search large spaces of candidate solutions. We assume the initial parameter values (μ, K, c, α, p) = (1, 1, 1, 1, 1) and estimate their optimal values in the ranges of 0.0001–1, 0.1–100, 0.01–10, 0.01–10, and 0.01–10, respectively.

We set M c  = 4.5 in order to remove the seismicity of small earthquakes from the Gutenberg–Richter law (Gutenberg and Richter 1944). As a basis for the M c value, Fig. 1 illustrates the relationship between the number of earthquakes and earthquake magnitudes for the world in the ANSS comprehensive catalogue. The value of M c  = 4.5 is the same as that in a previous study estimating the ETAS parameters from the ANSS catalogue (Ide 2013).

Fig. 1
figure1

Earthquake numbers versus magnitudes for the world in the ANSS comprehensive catalogue. The vertical broken line represents magnitude 4.5, which is equal to the threshold value obtained by removing smaller earthquakes from the Gutenberg–Richter law

The study period to estimate the ETAS parameters is from April 2002 to July 2016, and the spatial range is 10 degrees of latitude/longitude, which is the same as the GRACE data.

We perform correlation analysis for the amplitudes of the annual gravity changes \(\sqrt {C^{2} + D^{2} }\) and the background seismicity rate μ. As described in the introduction section, our aim is to clarify the relation between gravity change and occurrence of small earthquakes. Thus, we exclude the areas experienced large earthquakes of magnitude greater than 7.5 in the study period. This deselection is also useful to avoid (aseismic) stressing effects of postseismic deformation within the areas, probably increasing the background seismicity rate μ (Llenos et al. 2009).

Results

Figure 2 shows global distribution of the annual gravity change used in this study. We refer to Bird (2003) for locations of plate boundaries. Table 1 shows the results for the amplitude of the annual gravity change.

Fig. 2
figure2

Distribution of the amplitude of annual gravity change (as equivalent water thickness) in this study. Areas of no data are overlaid with a dark-brown color. Note that we exclude the areas experienced large earthquakes of magnitude greater than 7.5 in the study period. The black stars represent epicenters of the large earthquakes. The blue broken lines show plate boundaries compiled by Bird (2003)

Table 1 Estimated amplitude of the annual gravity change and their 95% confidence intervals, as equivalent water thickness (units: cm), within each spatial area

There are two kinds of the results of the ETAS parameter estimation. One is based on the quasi-Newton method (hereinafter called QN method). In case of this method, we evaluate 95% confidence intervals by calculating inverse of Hessian matrix. The other is based on the differential evolution method (hereinafter called DE method), where we are not able to evaluate confidence intervals. Table 2 exhibits the estimation results of the background seismicity rate μ. We confirm that the results of QN method and DE method are almost the same; therefore, we rely on the estimated values.

Table 2 Estimated background seismicity rate μ by QN method (with 95% confidence intervals) and by DE method

Figure 3 compiles the estimated amplitude of the annual gravity change and the background seismicity rate (by QN method). We find a roughly linear relationship between them. The correlation coefficient is 0.51 with a p value of 1.7%. Thus, there is moderate positive correlation between the annual gravity amplitudes and the background seismicity rates. Additionally, we examine correlation between the amplitudes of the annual gravity changes and earthquake numbers (including aftershock effects) in Table 2. In this case, the correlation coefficient is 0.23 with a p value of 31%, which is not a reliable correlation. It is necessary to estimate the background seismicity rate for extracting features of earthquake occurrence without aftershock effects.

Fig. 3
figure3

Amplitude of the annual gravity change versus the background seismicity rate (by QN method). The error bars represent the 95% confidence intervals

Besides, we check a relation between the background seismicity rates and the plate convergence rate (Ide 2013). Figure 4 illustrates our results and the empirical relation proposed by Ide (2013). We find that our results roughly follow the empirical relation but their correlation is not strong (correlation coefficient = 0.20). This may be due to the difference of the data set. For example, we did not investigate the areas experienced large earthquakes in the study period, to avoid the effects of postseismic deformation.

Fig. 4
figure4

Relation between the estimated background seismicity rates and the plate convergence rates in Table 2. The broken line shows an empirical relation proposed by Ide (2013)

Discussion

Examination of effects of pore pressure and surface load

What causes the positive correlation between the annual gravity amplitudes and the background seismicity rates? As described in the introduction section, the relation between gravity change and occurrence of small earthquakes may reflect the earthquake triggering due to water movement around the surface. The possible two mechanisms are friction reduction by pore-fluid pressure increase and elastic stress change due to surface load on faults.

First, we discuss the former effect of pore pressure increase, associated with fluid infiltration from the surface through high-permeability pathway (e.g., fault). This possible triggering effect should be stronger for shallower earthquakes. In order to investigate this point, we vary the depth range of the earthquakes for the correlation study. Our results in the previous section were based on the earthquakes whose focal depths were shallower than 30 km. We test another threshold value of the depth and check the correlation coefficient between the annual gravity amplitude and the background seismicity rate. Figure 5 shows the results. Unexpectedly, we find that the correlation coefficient does not increase for a smaller threshold value of the depth. We infer that effects of the pore pressure increase hardly trigger the shallow earthquakes.

Fig. 5
figure5

Variation of the correlation coefficient between the annual gravity amplitude and the background seismicity rate with changing the depth threshold for shallow earthquakes

Next, we examine the latter effect of elastic surface load. As equivalent water thickness, the mass estimated from the GRACE data was on the order of 1–10 cm (Table 1). If we assume that the mass concentrates on the surface for simplicity, we can evaluate hydrostatic pressure of the mass as source of surface load. From the following parameters: 1000 kg/m3 for water density, 9.8 m/s2 for gravitational acceleration, and 0.1 m for water thickness, we obtain the hydrostatic pressure about 1 kPa on the surface.

Furthermore, we estimate degrees of Coulomb stress changes (dCFF) on subduction reverse faults due to the surface load, using a two-dimensional Green’s function in an elastic half-space (Poulos and Davis 1974). Figure 6 illustrates normalized results of dCFF for left-dipping reverse faults due to unit surface loads. Positive surface loads approximately cause − 0.1 to − 0.7 times stress changes on reverse faults beneath the load area, which should lead to restraining earthquakes. For instance, when the surface load by water mass movement is about 1 kPa as estimated above, the dCFFs on reverse faults are approximately from − 0.1 to − 0.7 kPa. It means that the stress changes on underground faults would be lower than 1 kPa. This value is at least one-order smaller than a typical value of earthquake triggering by elastostatic stress change in the literature (Hardebeck et al. 1998; Freed 2005).

Fig. 6
figure6

Normalized Coulomb stress changes (dCFF) for left-dipping reverse faults due to unit surface loads at horizontal positions from 0 to 1. We assume frictional coefficient = 0.6. The horizontal and the vertical axes represent normalized horizontal position and normalized depth, respectively. The upper figure shows a result for the dip angle = 10°, and the lower figure shows for the dip angle = 45°

However, not only our study but also a recent study about regional seismicity in California (Johnson et al. 2017) revealed that seasonal water storage, causing stress change on faults as small as 1 kPa, modulated seismicity rates. Recently, on the basis of seismicity analysis (of tremors) about tidal responses, Ide and Tanaka (2014) and Tanaka et al. (2015a) suggested exponential dependence of stress changes on fault slip rates. This corresponds to the rate and state friction framework (Dieterich 1994) based on laboratory rock experiment. Using the rate and state framework, Beeler and Lockner (2003) predicted correlation between earthquake occurrence and periodic stress only in cases of longer periods than earthquake nucleation time. Our result may correspond to their prediction, since the period of the stress changes in our study is annual. Moreover, Tanaka (2014) implied a resonance effect of periodic force on seismicity.

Not clear relation between annual gravity phase and seismicity

We have discussed the possible correlation between the annual gravity “amplitude” and the background seismicity. Here, in the light of “phase” of the annual gravity change, which may reflect the surface load effect on seismicity, we show monthly changes in the gravity as equivalent water thickness and the earthquake number from April 2002, at a grid of (longitude, latitude) = (275°, 5°) and at an adjacent grid of (longitude, latitude) = (275°, − 5°), in Fig. 7. In case of the former grid (Fig. 7a) with a larger amplitude of the annual gravity change, months with many earthquakes tend to be during periods of negative amplitude of the fitted sinusoid. Namely, 6 of 8 months with 5 or more earthquake occurrence, where 5 is a two-sigma threshold of earthquake numbers per month, are in negative amplitude of the fitted sinusoid. The tendency is not apparent in case of the latter grid (Fig. 7b) with a smaller amplitude of the annual gravity change. This fact agrees with the negative dependence of the surface loads on the dCFFs, as estimated in the previous paragraph. However, from a statistical point of view, we were not able to reject a null hypothesis under the assumption of random occurrence. At this moment, we state that the relation between the “phase” of the annual gravity changes and seismicity is unclear.

Fig. 7
figure7

Example of monthly changes in the gravity as equivalent water thickness and the earthquake number from April 2002. The black line shows the gravity data, and the red broken line does the fitted curve using Eq. (1). The vertical gray bars represent the earthquake number. The upper figure a shows the results at a grid of (longitude, latitude) = (275°, 5°), and the lower b shows at an adjacent grid of (longitude, latitude) = (275°, −5°) for comparison

Other possible mechanisms behind the correlation

Our analyses in this study targeted at subduction zones. We have two problems. First, other tectonic factors, possibly contributing the background seismicity rates (e.g., Nishikawa and Ide 2015), might contaminate the effects of periodic stress perturbation. Thus, inland areas may be more suitable for analyzing the effects of the periodic water mass movements. Since the global seismicity catalogue does not contain sufficient numbers of small (but over M 4.5) inland earthquakes, we did not analyze the inland areas in this study. Second, we did not consider atmospheric and oceanic load effects. Annual changes of atmospheric pressure can be on the order of 1 kPa (Ohtake and Nakahara 1999), comparable to that by the water mass movements in this study. Annual changes of ocean bottom pressure can be also as large as 1 kPa (Tanaka et al. 2015a). These load effects may also modulate seismicities. The above problems would be the focus of our future work.

Conclusions

Through correlation analysis, we find a moderate positive correlation between the amplitudes of the annual gravity changes and the shallow background seismicity rates at the worldwide subduction zones excluding the source areas of large earthquakes. This implies that annual water cycle can activate shallow earthquakes, although the surface load elastostatic stress changes are on the order of or below 1 kPa, as small as the regional case in the previous study.

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Authors’ contributions

YM performed the data analyses and wrote the paper. KY helped the analyses and discussed the results. Both authors read and approved the final manuscript.

Acknowledgements

We used generic mapping tools (Wessel et al. 2013) to draw maps. The time-variable gravity and seismicity data were provided by JPL and USGS. We acknowledge support from the Japan Society for the Promotion of Science (JSPS) KAKENHI, Grant Numbers JP16K17791 and JP16H06477. Kyohei Yamada was formerly at Department of Geosciences, Shizuoka University, 836, Ohya, Surugaku, Shizuoka 422–8529, Japan.

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Correspondence to Yuta Mitsui.

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Keywords

  • GRACE
  • Gravity change
  • ETAS model
  • Background seismicity rate
  • Surface load
  • Pore pressure