Abstract
In this study, we analyzed the performance of a preliminary three-dimensional (3D) velocity model of the Eastern Caucasus covering most of the Azerbaijan. The model was developed in support to long-period ground motion simulations and seismic hazard assessment from regional earthquakes in Azerbaijan. The model’s performance was investigated by simulating ground motion from the damaging Mw 5.9, 2012 Zaqatala earthquake, which was well recorded throughout the region by broadband seismic instruments. In our simulations, we use a parallelized finite-difference method of fourth-order accuracy. The comparison between the simulated and recorded ground motion velocity in the modeled period range of 3–20 s shows that in general, the 3D velocity model performs well. Areas in which the model needs improvements are located mainly in the central part of the Kura basin and in the Caspian Sea coastal areas. Comparisons of simulated ground motion using our 3D velocity model and corresponding 1D regional velocity model were used to locate areas with strong 3D wave propagation effects. In areas with complex underground structure, the 1D model fails to produce the observed ground motion amplitude and duration, and spatial extend of ground motion amplification caused by wave propagation effects.
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1 Introduction
The Eastern Caucasus region has a long history of damaging earthquakes (Kondorskaya and Shebalin 1977; Storchak et al. 2013). The high seismicity, rapid population growth, and a recent increase in civil, industrial, and infrastructure construction suggest for significantly increased seismic risk in the region. A necessary step in assessing seismic risk is to estimate the hazard, i.e., a quantitative estimate of the expected ground motion during a specified time window. A variety of methods for estimating seismic hazard exist, but all require a good knowledge of wave propagation and attenuation.
In this study, we test the performance of a preliminary regional 3D velocity model developed by Gok et al. (2011) by simulating ground motion in the period range of 3–20 s from the Mw 5.9, May 7, 2012 Zaqatala earthquake, recorded in the Eastern Caucasus (Fig. 1). The simulated ground motion was compared with observed ground motion at seismic stations in the Azerbaijan region. Maps of simulated ground motion were then used to investigate 3D basin effects in the Azerbaijan region, and identify areas, where the 3D velocity model needs further refinement.
Seismic hazard assessment in regions with limited strong motion data and complex structure requires accurate 3D seismic velocity models that can be used to estimate ground motion amplification due to wave propagation effects. Hybrid methods that combine low- and high-frequency approaches for simulating broadband ground motion have produced reliable synthetic data that are useful to seismic hazard assessment and building response analysis (e.g., Pitarka et al. 2000; Graves and Pitarka 2010). Simulations of strong ground motion at regional distances (>200 km) often rely on 1D velocity models that are mostly calibrated for travel time and long-period surface wave amplitude (e.g., Pulido et al. 2015). 1D models tend to overestimate the amplitude and duration of long-period waves (Dreger et al. 2015; Rodgers et al. 1999). The absence of 3D structural heterogeneity in 1D velocity models can cause overestimation of the so-called wave trapping effect, or ringing effect, which typically generates dispersive surface waves with extremely long duration. In contrast, 3D models allow for realistic modeling of wave scattering caused by wave conversions, reflections, and focusing and defocusing in heterogeneous underground structures. Earthquake ground motion modeling requires crustal models with high spatial resolution, especially in basins areas with sharp velocity contrast and large multi-scale structural variability.
2 Tectonics, Underground Structure, and 3D Velocity Model
The Azerbaijan region lies in a complex and relatively poorly understood tectonic setting of Eastern Caucasus. The northern region is dominated by shortening along the Greater Caucasus, which is an area of complex active shortening at both crustal and deeper structures (e.g., Forte et al. 2010). To the east is the Caspian Sea, which is underlain by two different basins: the South Caspian basin which has more than 10 km of sediments and the North Caspian basin which has a thinner set of sediments on continental crust. Between the two basins is the Absheron structure, a zone of possible incipient subduction characterized by both crustal and intermediate depth seismicity (Jackson et al. 2002). The southern part of the territory extends over the Lesser Caucasus and northern edge of the Iranian plateau. Between is the Kura Depression, with sediments up to 8 km thick that appears to be gradually subsumed under the Greater Caucasus. Below the sediments are meta-volcanic layers that resemble the surface geology of the Lesser Caucasus.
Various geophysical studies have examined the deep structure and velocity structure of the region. These include refraction and reflection profiles, deep boreholes, and passive seismic studies using earthquakes, receiver functions, and ambient noise. For this study, we used a smoothed and interpolated version of the crustal structure inferred by Gok et al. (2011), which was based on a joint inversion of receiver functions and surface waves, using both ambient noise and earthquake recordings measurements. The two sets of measurements were made using data from 14 broadband stations of the Azerbaijan network which provides a good stations coverage of the area. The Moho and basement depths in Gok et al. model were checked for consistency with other data where available, such as deep seismic sounding (DSS) measurements and borehole data at the 8 km deep Saatli well. Other studies of the underground structure based on active seismic sources or shallow borehole data cover very small areas.
Figure 2 shows maps of depth to basement, depth to shallow crustal layer, and Moho boundary extracted from model. In this figure, also shown are the surface topography and the stations location. The geometry of these boundaries as well as seismic velocities for each layer was used to generate a 3D regional velocity model. The seismic parameters assigned to each layer are shown in Table 1. We believe that this model captures the major crustal features, although discrepancies do exist. For example, in our model, the basement under Kura slopes down towards the Caspian, whereas there is evidence that an increase in basement elevation extends parallel to the Caspian coast (e.g., Kadirov 2000). However, full consideration of all available geologic and geophysical data is beyond the scope of this study which is mainly focused on long-period ground motion modeling.
3 Simulation of the Mw 5.9, 2012 Zaqatala Earthquake
We tested the 3D velocity model by simulating ground motion in the period range 3–20 s, recorded during the Mw 5.9, 2012 Zaqatala earthquake. The earthquake occurred on May 7, 2012 at 04:40:30 GMT in the Zaqatala region of Azerbaijan. The earthquake caused severe damage to thousands of residential houses in the epicentral area. It occurred on a thrust fault in the Greater Caucasus Range-Front fault system, and was followed by two large aftershocks of Mw 5.3 and Mw 4.8, respectively, that caused an additional damage. The earthquake was well recorded by 14 broadband seismic stations installed throughout the region and on various geological conditions. The particular location of the earthquake near the northern edge of the Kura basin and its thrust mechanism made it an ideal source for exciting the basin response and basin generated waves that travel across the region, therefore carrying information not only about the source but also about the subsurface structure. The recorded ground motion was simulated by a parallelized computer program based on a finite-difference method of the fourth-order accuracy in space (SW4) (Petersson and Sjogreen 2012). SW4 is capable of modeling non-flat surface topography with good accuracy and unelastic wave propagation, as well.
In our simulations, we included the surface topography and used a kinematic model of earthquake rupture. The rupture propagates bilaterally on a 12 km × 6 km planar fault. The strike and dip angles of the fault plane are 108° and 82°, respectively, and the slip rake angle is 88°. The earthquake focal mechanism was obtained using moment tenser inversion of regional waveforms using Ichinose’s technique (e.g., Ichinose et al. 2003). The slip distribution of the rupture scenario considered here is dominated by a single asperity in which the slip is 42 cm (Fig. 3). As it will be shown later, because of the relatively small size of the earthquake, the details of the slip distribution in the rupture model have insignificant effects on the computed long-period ground motion. The rupture velocity is computed as 80 % of the local shear wave velocity. We used a Gaussian slip velocity function with a constant duration of 0.85 s estimated using the empirical rupture model of Somerville et al. (1999). The rupture initiation depth is 15 km, and the seismic moment of the earthquake is 6.72e+17 Nm.
The finite-difference computation was performed using a minimum grid spacing of 300 m which ensures sufficiently accurate wave propagation modeling at frequencies up to 0.3 Hz. The comparison between the simulated and recorded time histories of ground motion velocity, band-pass filtered at 0.05–0.3 Hz is shown in Fig. 4. A more quantitative assessment of goodness-of-fit is shown in Fig. 5. Due to its poor quality, the record at ZKT, the nearest station to the epicenter, was not used in the comparison. In general, the simulation reproduces the amplitude and duration of the recorded ground motion at several sites. The largest misfit is observed at stations SIZ and QUB for which the E–W component of ground motion is largely underestimated. Both sites are located near the basin edge where wave focusing caused by basin edge geometry (e.g., Pitarka et al. 1998) is expected to be more pronounced.
We quantified the overall comparison between recorded and simulated ground motion using goodness-of-fit measures for 5 % damped horizontal spectral acceleration (Fig. 5). The ground motion acceleration time history at each station was obtained by computing the time derivative of the velocity time history. For an individual station, the residual r(P i ) at each period P i is given by r(P i ) = ln[SAO(P i )/SAS(P i )], where SAO(P i ) and SAS(P i ) are the observed and simulated spectral acceleration values, respectively. The model bias is obtained by averaging the residuals for all stations and the horizontal component RotD50 (Boore et al. 2006), at each period. A model bias of zero indicates the simulation, on average, matches the observed ground motion level. A negative model bias indicates over-prediction, and a positive model bias indicates the under-prediction of the observations. The simulated ground motion has no significant bias over the period range 3.5–10 s, indicating that the 3D model adequately captures the main characteristics of ground motion response at sites located in and outside the Kura basin.
4 Ground Motion Sensitivity Analysis
We performed several simulations of the Zaqatala earthquake to address the sensitivity of simulated ground motion to source and velocity models. We looked at the ground motion difference between a double-couple point source and kinematic fault rupture model. Because of the limited energy generated at long periods, it is expected that details of the rupture process of small and intermediate size earthquakes have a negligible effects on long-period ground motion (>3 s), especially at long distances (longer than several times the fault length). We tested this hypothesis by comparing simulated ground motion obtained with a kinematic slip model and double-couple point source model of Zaqatala earthquake. We used the same seismic moment, mechanism, depth, and slip velocity function for both source models. The comparison of time histories of simulated ground motion velocity, band-pass filtered at 0.05–0.3 Hz, is shown in Fig. 6. The two models produce ground motion with similar amplitudes, with the point source model producing slightly lower ground motion. The difference in ground motion amplitude remains almost the same at all stations suggesting that the discrepancy is not related to wave propagation effects but rather source effects. In the extended rupture model, the rupture propagates through a relatively large area, thus producing rupture directivity effects. The thrust mechanism generates upward directivity. Such effects can explain the observed difference between the point and extended source. The relatively small difference in ground motion between the two source models suggests that the point source model is valid for modeling intermediate size earthquakes (M ~ 6) at long epicentral distances.
A common practice in seismic hazard assessment in areas with unknown 3D underground structure is the use of 1D velocity models in ground motion estimates. 1D velocity models, usually calibrated for travel time and surface wave amplitude, do not guaranty high-quality ground motion modeling in a broad frequency range. The main drawback of ground motion simulated with 1D velocity models is the enhanced band limited amplification of coda waves controlled by the resonant frequency of individual flat layers. In general, 1D models tend to produce larger than recorded long-period ground motion (Pitarka et al. 2014; Dreger et al. 2015). Here, we compare ground motion simulated with the 3D model and the corresponding 1D local velocity model, as shown in Table 2. To avoid mixing source effects, associated with rupture propagating through a complex structure, and wave propagation effects, in both simulations, we used the double-couple point source model of the earthquake. Both models include surface topography. The comparison of simulated ground motion is shown in Fig. 7. It is evident that at basin sites, including BRD and KDR, the 1D model does a poor job at producing basin-induced waves which are correctly produced by the 3D model. In addition, at non-basin and distant sites, such as ATG, PQL, and SIZ, the wave trapping effect caused by the 1D model produces ground motion with unrealistic amplitude and duration. Maps of horizontal peak ground motion velocity, computed with the 1D and 3D velocity models, shown in Fig. 8, give a clear picture of the spatial extend of the effects of the 3D underground structure on ground motion amplitude. The contrast in terms of peak ground motion between the two models is strong in the Kura basin and along the Kaspian Sea coast.
We used selected snapshots of computed vertical component of ground motion velocity, shown in Fig. 9, to illustrate the contributions of the source and wave propagation effects on ground motion amplitude. First, due to the thrust focal mechanism, most of the source energy is directed toward northeast and southwest directions. Second, waves propagating in deep valleys along the Greater Caucasus mountain range and Kura basin are delayed and amplified due to lower velocity in the sedimentary layers. Third, and most importantly, the basin underground structure amplifies long-period surface waves and deflects their propagation direction from southwest to east. Significant wave reverberations are also seen along the Kaspian Sea coast. The fourth snapshot taken 264 s after the rupture initiation shows tremendous basin reverberations in the deepest part of the Kura basin. These basin-trapped waves greatly increase the amplitude and duration of coda waves.
5 Conclusions
In this study, we tested the performance of a preliminary 3D velocity model (Gok et al. 2011) in simulations of long-period ground motion in the Azerbaijan area and demonstrated the importance of considering 3D underground structure in estimating long-period ground motion response to distant earthquakes. The spatial distribution of the seismic stations used in developing the model limits its resolution, especially in areas with complex underground structure and in the central part of the Kura basin where the basin depth exceeds 6 km. The 3D velocity model performed relatively well in simulations of ground motion from the Mw 5.9, 2012 Zaqatala earthquake recorded by the broadband Azerbaijan Seismic Survey network. Sensitivity analysis of ground motion to earthquake source models suggests that for intermediate size earthquakes (M < 6) in the Greater Caucasus Range-Front fault system, long-period (>3 s) ground motion computed in the Kura basin is not sensitive to fault rupture details. Therefore, simple double-couple point source modeling of small and moderate size earthquakes in the region can produce reliable results. The comparison between computed and recorded ground motion in the frequency range of 0.05–0.3 Hz suggests that the 3D model used here lacks resolution and need improvements in the central part of the Kura basin, and in particular in the Kaspian Sea coast where the simulation of the Zaqatala earthquake largely underpredicts the effect of basin edge on ground motion velocity.
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This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344, LLNL-JRNL-679075.
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Pitarka, A., Gok, R., Yetirmishli, G. et al. Ground Motion Modeling in the Eastern Caucasus. Pure Appl. Geophys. 173, 2791–2801 (2016). https://doi.org/10.1007/s00024-016-1311-2
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DOI: https://doi.org/10.1007/s00024-016-1311-2