Abstract
The 2003 Boumerdes earthquake occurred in the north of Algeria and caused significant amounts of damage in the cities of Boumerdes and Algiers. This study aims to simulate strong ground motion of the mainshock and aftershock of this earthquake by using empirical Green’s function method (EGFM). The obtained source model of the main shock called strong motion generation areas (SMGA) is nearly compatible with the asperities derived from the waveform inversion results. A good agreement is shown between the observed and simulated ground motions in the frequency range of 0.25–10 Hz, which is of interest in almost all engineering applications. Besides, EGFM is successfully used to define the source model for the Mw 5.7 aftershock by comparing the simulated to the recorded motions at two near stations. Source parameters of the Mw 6.8 mainshock and the Mw 5.7 aftershock, such as the asperities area and the rise time, are compared with scaling laws and show good agreement with previous published studies for crustal earthquakes. Consequently, this study shows that the Irikura recipe for predicting strong ground motion in Algeria could be an effective tool for simulating future large earthquakes characterized by long return period by using records of small earthquakes combined with source models derived from scaling relationships.
1. Introduction
Natural disasters, namely earthquakes, represent a major challenge for the urban and economic development of a region and a country. If it is not possible to act on the seismic hazard, that is to say on the magnitude and occurrence of earthquakes, it is however possible to reduce the seismic risk by seismic risk prevention. The evaluation of seismic hazard and the preparation of scenarios for future earthquakes is the first step in the prevention of seismic risk. Simulation of ground motion is an important tool to in reproducing ground motion movement of past earthquake or to simulate future earthquakes that could strike the region.
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The empirical Green’s function method (EGFM) is a powerful method for strong ground motion simulations that uses small earthquake records at the same site to simulate a large earthquake. This works because the site and the path effects are already contained in the small event waveforms recorded at the same site from the region of the hypocenter. Miyake et al. (2003) defined the strong ground motion generation area, which is a portion of the fault rupture surface with a large and uniform slip velocity area that is nearly equivalent to the asperity area (the large slip region). In this study, we attempted to define a source model and simulate the ground motion using the EGFM for two events: the Mw 6.8 mainshock and the Mw 5.7 event of the 2003 Boumerdes earthquake. In addition, we compared the source parameters obtained for the two events with scaling laws prepared in other regions of the world to use them for seismic hazard assessments of North Africa. This paper aims to apply the EGFM to reproduce the strong ground motion of this event at a different site.
Several destructive earthquakes have struck the northern of Algeria. In fact, this region resides on the boundary of the African and Eurasian plates, and its active tectonics results from the collision between these two plates. The strongest earthquakes in the last century have been Orléansville on 9 September 1954 (M = 6.7) (Rothé, 1955), El Asnam on 10 October 1980 (M = 7.3) (Ouyed et al., 1980), Tipaza on 29 October 1989 (M = 6.0) (Meghraoui, 1991), Ain Temouchent on 22 December 1999 (M = 5.8) (Yelles et al., 2004), and Boumerdes-Zemmouri on 21 May 2003 (M = 6.8) (Ayadi et al., 2003). The latter was one of the most destructive earthquakes that has occurred and caused a large area of damage in the city of Boumerdes and the eastern part of Algiers with more than 2300 casualties and the destruction of more than 10,000 houses (Ayadi et al., 2003). Being nearly the largest ever recorded earthquake in North Africa, the strong ground motion of the 2003 Boumerdes earthquake is important to study in detail to understand how buildings performed during the earthquake and why they failed, particularly near the hypocenter area.
The application of the EGFM for the 2003 Boumerdes earthquake has the advantage to reproduce the recorded seismic movement and thus to validate the source model and to compare it with the source parameter’s scale laws established for earthquakes of other regions of the world. In addition, it allows simulating the seismic movement in the near field in which no seismic recordings are available and therefore to better understand the origin of the major damage that has occurred in the near field
2. Strong Ground Motion Simulation Of The Mw 6.8 Boumerdes Earthquake
2.1 Strong Motion Data
In this study, we used strong motion records obtained from the Algerian national accelerograph network monitored by the National Center of Applied Research in Earthquake Engineering (CGS; www.cgs.dz). Figure 1 shows the locations of those stations together with the epicenters of the mainshock and aftershocks used in this study. All stations are located on the hanging wall side extending from 30 km to 180 km from the epicenter. Therefore, we do not have much near-field strong motion data in the damaged area of Boumerdes and the eastern part of Algiers.
Of the many aftershock records available, only two or three aftershocks have an available focal mechanism solution and were recorded at nearly all stations; therefore, they were selected as the empirical Green’s functions. Table 1 shows the selected aftershocks for this study, their characteristics, and the stations at which they were recorded. The records of the Mw 4.3 aftershock at 17:42:24 on 2 February 2004 were selected for the empirical Green’s functions because the focal mechanism was close to that of the mainshock. This event was recorded by several stations, except for the TZO, MLA, and ADF stations, where we used Mw 4.7 on 1 October 2004 as the empirical Green’s function; this event has a focal mechanism that is different from that of the mainshock.
2.2 Source Modeling of Strong Motion Generation Areas
Several studies have determined slip distribution models of the 2003 Boumerdes earthquake using different types of data (e.g., geodetic, teleseismic, and strong motion). All of these published rupture models (Meghraoui et al., 2003; Delouis et al., 2004; Semmane et al., 2005; Belabbès et al., 2009; Santos et al., 2015) show the existence of at least two asperities: the first asperity is located northeast of the hypocenter where the maximal displacement reaches 3 m and the second asperity is located southwest of the hypocenter in a shallow region (Figure 2).
Asperities are regions that have large slip relative to the average slip in the rupture area (Somerville et al., 1999). In addition, it has been shown that strong ground motion is primarily produced by large slips occurring at asperities (Miyake et al., 2003). Therefore, synthetic ground motions can be calculated assuming that ground motions are only generated within the strong motion generation areas, which are redefined based on the asperity location and the area information (Kamae and Irikura, 1998; Miyake et al., 2003).
We fixed the following fault parameters: the epicenter is located at 36.846° N and 3.660° E, the strike, dip, and rake angles are 64°, 50°, and 97°, respectively, and the hypocenter depth is 8 km (Santos et al., 2015).
The initial source model for the ground motion simulation was established based on the slip distribution shown in Figure 2. Two strong motion generation areas (SMGAs) corresponding to the two asperities were constructed for this model. SMGA1 corresponds to the first asperity located southwest of the hypocenter, and SMGA2 corresponds to the second asperity located northeast of the hypocenter.
The parameters N and C, which are the number of subfaults at each asperity and the stress drop ratio, respectively, were obtained from the acceleration amplitude ratio of the small and large events. Figure 3 shows the amplitude ratio for the two stations EDB and TZO located west and east of the hypocenter, respectively. The ratio of the corner frequencies of the small and large events (fa and fo, respectively,) gives an estimate of N, while the ratio of the seismic moments (g) gives C × N3; then, we can estimate the values of C and N as an initial guess for the EGFM.
The final source parameters, such as N, C, the starting point rupture for each SMGA, and the rise time, were obtained by applying a trial-and-error forward modeling method that produced a good match between the observed and simulated ground motions. It has been shown that waveforms at the TZO station were primarily dominated by SMGA1, while waveforms at the CGS, EDB, and KTA stations located west of the hypocenter were dominated by SMGA2. Figure 4 shows the source model composed of two strong motion generation areas for the Mw 6.8 Boumerdes earthquake, and Table 2 shows all the parameters used for our simulation. After trial and error, we selected a rupture velocity of 2.8 km/s corresponding to 90% of the shear wave velocity (3.1 km/s).
2.3 Results and Discussion
Figure 5 shows a comparison between the simulated and observed waveforms of the mainshock in terms of acceleration, velocity, and displacement in the frequency range of 0.25–10 Hz. The Fourier amplitudes and the response spectra comparison between the recorded and simulated ground motions are shown in Figure 6.
The best source model was obtained by fitting the synthetic accelerations, velocities, and displacement waveforms to the observed ones. Seismic wave propagation and site amplification effects on the strong ground motion were explicitly taken into account by considering the aftershocks recorded at the same stations as the empirical Green’s functions.
The EGFM was applied using the Mw 4.3 aftershock for all stations, except TZO, where we used an Mw 4.5 aftershock event as the Green’s function. The quality of the fit between the simulated and observed waveforms was quantified via a visual inspection, and an acceptable visual match was obtained for all stations, except CGS and KTA, which are located 60 km from the hypocenter and where we can show that the accelerations obtained are underestimated compared to the observed ones. This could be due to the inadequacy of the Green’s function used (the location and focal mechanism), or it may be due to problems with the localization of the fault plane.
Large displacements at later phases for the EDB, CGS, and KTA stations could be due to the surface waves generated along the path due to the presence of the quaternary Metija Basin (Laouami and Slimani, 2013). These displacements were roughly reproduced by the EGFM.
The TZO station is 40 km from the hypocenter in the eastern region, and there is only one Mw 4.5 aftershock that has a record available for use as an empirical Green’s function. We found that the strong ground motion was produced primarily by SMGA1. The rupture starting point was assumed to be close to the hypocenter. Conversely, the EDB, CGS, and KTA stations were primarily influenced by SMGA2, which is located northeast of the hypocenter.
Waveforms at the EDB station located 40 km from the hypocenter show large values of peak ground velocity (PGV) for the two components and reach a value of PGV = 41 cm/s for the north/south component with a pulse-like shape with a period of approximately 3–4 s. This effect was moderately reproduced by the EGFM and is related to rupture propagation at the second asperity (SMGA2) located less than 25 km from this station (a directivity effect). A peak ground acceleration of 0.5 g was recorded at this station in both directions. This value was obtained by our EGFM simulation in both directions, which reveals important site effect amplifications. As for the waveform comparisons at the CGS and KTA stations, there is a possibility of the source model and asperity locations based on the slip inversion result are sensitive, and there are still room to be improved.
Other source parameters, such as N, C, and the rise time, were estimated using the EGFM. Broadband ground motion simulations were performed for stations located primarily west of the hypocenter, except for TZO, which is located to the east. The results show good agreement between the simulated and observed motions in the frequency range of 0.25–10 Hz, which is of interest in nearly all engineering applications. Waveforms recorded at a station located in Dar el Beida, 40 km from the hypocenter, show a clear forward directivity pulse with a PGV of 41 cm/s at a dominant period of 3–4 s corresponding to rupture propagation through the second asperity located in the southeastern part of the surface rupture.
3. Strong Motion Simulation Of The Mw 5.7 Boumerdes Aftershock Earthquake
We applied the EGFM to simulate the Mw 5.7 event that occurred on 27 May 2013, which was one of the largest aftershocks of the mainshock. This event was recorded by two stations: CRD (Boumerdes) and ST1 (Keddara). We set the fault plane solution of this aftershock using the CMT solution. The actual fault plane considered in this study has strike, dip, and rake angles equal to 68°, 24°, and 92°, respectively.
Table 3 shows the characteristics of the aftershocks used as the empirical Green’s functions. The location of the Mw 4.3 aftershock is very close to the CRD station (less than 5 km), therefore we decided to use, as the empirical Green’s function, the Mw 4.7 earthquake event, which has a similar focal mechanism and is located at the same distance as the Mw 5.7 event from the station (Figure 7). We used the same rupture velocity and shear wave velocity for the simulation of the Mw 5.7 event.
The source spectral ratio fitting method was used to estimate the parameters N and C that correspond to the two aftershocks used for the CRD and ST1 stations (Table 3). The parameters of the strong motion generation area were estimated using forward modeling by fitting the simulated waveforms to the observed waveforms. Table 4 shows all the parameters used for our simulation. The size of each subfault is 1.4 km × 1.2 km; therefore, the strong motion generation area is estimated to be 5.6 km long × 4.8 km wide (Figure 8). The starting point is assumed to be the hypocenter location. There are a lot of uncertainties about the SMGA locations, N and C parameters, starting point, rise time. This is why we do not obtain the exact same values for source parameters to simulate acceleration, velocity, and displacement. Currently, the waveform comparisons were done visually and the results show good agreement for some stations. For other stations, there are still some works to check the source model as well as Green’s functions to obtain a better source model for strong ground motion simulation of the 2003 Boumerdes earthquake sequence. Figure 9 shows the waveform fittings for the two stations in terms of acceleration, velocity, and displacement in the frequency range of 0.25–10 Hz. The overall fit is very good for the two stations.
4. Source Scaling
Based on the results of the empirical Green’s function simulations, we investigated the source scaling properties of the Mw 6.8 mainshock and the Mw 5.7 event for the 2003 Boumerdes earthquake by comparing the estimated source parameters with the empirical source scaling relationship for crustal earthquakes proposed by Somerville et al. (1999) and Miyake et al. (2003). The scaling relationship of Somerville et al. (1999) was derived using the results of waveform inversions at frequencies less than 1 Hz, and that of Miyake et al. (2003) was derived using empirical Green’s function simulations in the frequency band between 0.2 Hz and 10 Hz.
A comparison was made in terms of the size of the strong motion generation area versus the seismic moment and in terms of the rise time for the strong motion generation area versus the seismic moment. For the Mw 6.8 mainshock, the total area of the two SMGAs used and the rise time were Sa = 130 km2 and T = 1.0 s respectively. For the Mw 5.7 aftershock, we obtained Sa = 30 km2 and T = 0.4 s. The results of the source scaling characteristic analysis are presented in Figure 10. We can clearly conclude that the source parameters obtained in this study in terms of the strong motion generation area and the rise time are in good agreement with the published scaling laws of Somerville et al. (1999) and Miyake et al. (2003) for crustal earthquakes.
5. Conclusions
The strong ground motion of the 2003 Boumerdes earthquake was simulated using the EGFM. The source model of the Mw 6.8 mainshock included two SMGAs that are nearly compatible with the asperities derived from the waveform inversions. Other source parameters, such as N, C, and the rise time, were estimated using the EGFM.
Broadband ground motion simulations were performed for stations located primarily west of the hypocenter, except for the TZO station, which is located east of the hypocenter. Waveforms recorded at a station located in Dar el Beida, 40 km from the hypocenter, show a clear forward directivity pulse with a dominant period of 3–4 s corresponding to the second asperity located in the southeastern part of the surface rupture.
In addition, the EGFM was used to simulate the strong ground motion of the Mw 5.7 aftershock recorded by two stations in the near field. The source model allowed for the simulation of ground motion waveforms that showed good agreement with the observed waveforms.
The source parameters, in terms of the strong motion generation area and rise time, obtained for the two events simulated in this study were compared to the scaling laws established for inland earthquakes by Miyake et al. (2003); we found that the obtained results conform to the scaling laws. Therefore, the use of a recipe (Irikura and Miyake, 2011) is possible for seismic scenarios with crustal earthquakes corresponding to active faults in North Africa by constructing source models based on scaling laws.
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