
Citation: | Liu YJ, Zhao XF, Wen ZP, Liu J, Chen B, Bu CY and Xu C (2023). Broadband ground motion simulation using a hybrid approach of the May 21, 2021 M7.4 earthquake in Maduo, Qinghai, China. Earthq Sci 36(3): 175–199,. DOI: 10.1016/j.eqs.2023.04.001 |
In this study, the broadband ground motions of the 2021 M7.4 Maduo earthquake were simulated to overcome the scarcity of ground motion recordings and the low resolution of macroseismic intensity map in sparsely populated high-altitude regions. The simulation was conducted with a hybrid methodology, combining a stochastic high-frequency simulation with a low-frequency ground motion simulation, from the regional 1-D velocity structure model and the Wang WM et al. (
On May 21, 2021, an M7.4 earthquake occurred in Maduo, Qinghai province, Northwest China, located on the top of the Tibetan Plateau (hereinafter referred to as the Maduo earthquake). The epicenter, as determined by the China Earthquake Network Center, was located at 34.59°N and 98.34°E. Figure 1 shows a surface projection map of the study area associated with the event. Notably, the Maduo earthquake caused much destruction in the high-altitude inland eastern Tibetan Plateau, resulting in many casualties and severe damage. In particular, in the epicentral region, infrastructure such as roads and bridges suffered considerable damage, and some bridges even collapsed (such as the Changmahe Bridge on provincial highway S219). Additionally, soil liquefaction occurred in the near-fault region.
The Maduo earthquake has generated widespread interest among the Chinese scientific community. The China Earthquake Administration released a shakemap of macroseismic intensity distribution for the Maduo earthquake. Ren JJ et al. (2022) conducted field observations and detailed measurements for the Maduo coseismic surface rupture and measured 114 offsets in situ. Their results indicate prominent surface breaks characterized by discontinuous shear faults, a dominantly left-lateral strike-slip motion with a maximum sinistral offset of ~2.7–2.8 m, and general offset of ~1.0–1.5 m. The west part of the Maduo surface rupture zone occurred along the Jiangcuo fault, and its east portion cut through some west-northwest-trending tectonics. To examine the source rupture characteristics of the Maduo earthquake, Wang WM et al. (2022) combined thirty far-field P waves, twenty-six SH waveforms, and INSAR coseismic displacement data into a joint inversion to construct the finite source fault model for the Maduo earthquake. Using seismic and geodetic data, Zhang X et al. (2022) investigated the spatiotemporal rupture complexity of the Maduo earthquake, and categorized it as a supershear event, with rupture propagating bilaterally towards both the west and the east. Using geodetic and seismic observations, Chen KJ et al. (2022) modeled the temporal evolution of fault slip during the earthquake, revealing that a slip-pulse ruptured 170 km along the fault system with a horizontal shear slip of up to 4.2 m. Liu CY et al. (2021) combined interferometric synthetic aperture radar, GPS, and teleseismic data to study the coseismic slip distribution, fault geometry, and dynamic source rupture process of the Maduo earthquake. Li Q et al.′s (2022) results indicate that the earthquake was a bilateral rupture event with asymmetric rupture velocities; the rupture velocity in the east was higher than that in the west and may have reached supershear velocity. Using 1-Hz GNSS displacement waveforms, GNSS static offsets, and SAR observations, Lyu MZ et al. (2022) indicated that this event spread bilaterally with asymmetric rupture velocities of 3.8 km/s to the southeast of the epicenter and 2.2 km/s to the northwest. Yue H et al. (2022) conducted a joint inversion for this earthquake and resolved a bilateral rupture process characterized by both super- and sub-shear rupture velocities.
However, some important issues still need to be addressed. The shakemap of the macroseismic intensity distribution for the Maduo earthquake has a very low resolution, with large uncertainty in the sparsely populated and high-altitude regions. This is because the epicentral region contains few buildings from which to infer macroseismic intensity. Therefore, alternative methods are needed, such as the strong ground motion method, to determine a more detailed shakemap of macroseismic intensity distribution. However, observing strong ground motion is made difficult by the infrequency of large earthquakes (Lee et al., 2003), especially in sparsely populated high-altitude regions. The Maduo earthquake occurred in the Bayan Har block along the eastern margin of the Tibetan Plateau, a sparsely populated area with a general elevation of 4100–4200 m. Unfortunately, the epicentral region of this event did not contain any strong ground motion stations, and no near-field strong ground motions were recorded for this large earthquake. This event only triggered 16 strong motion stations within the National Strong Motion Observation Network System (NSMONS) of China. Strong ground motions with a maximum peak ground acceleration (PGA) of 45.95 cm/s2 were recorded at station 63DAW, 175.47 km from the epicenter. However, most of these far-field recordings have no engineering significance. This lack of strong ground motion recordings has hindered direct estimations of ground shaking intensity, duration, and frequency which are required to understand earthquake behavior and to evaluate the performance of engineered structures during an earthquake. Therefore, simulated ground motions during the Maduo earthquake are required to conduct such estimations.
Deterministic physics-based, stochastic, or hybrid models can be used to numerically simulate ground motions. Physics-based models are attractive because they alleviate the need to explicitly prescribe the kinematic rupture process, which, in many instances, must be based on simplified assumptions and approximations (Graves and Pitarka, 2004, 2010). Unfortunately, the current realization of earthquake rupture dynamics is limited and suffers from a scarcity of direct observations and measurements, especially for those processes affecting the propagation of high-frequency ground motions (Graves and Pitarka, 2010). In contrast, stochastic models are generally simpler to generate and consequently are more convenient to use than deterministic physics-based models (Beresnev and Atkinson, 1997; Boore, 2003). Additionally, in many cases, these models are more accurate in simulating high-frequency ground motions. Alternatively, hybrid models can compute low- and high-frequency ground motions separately and then combine them to produce a single time series of shaking (Hartzell et al., 1999).
The hybrid broadband ground motion simulation method developed by Graves and Pitarka (2010) (hereafter referred to as the GP method) may provide useful insights into strong ground motions resulting from the 2021 M7.4 Maduo earthquake at regional and specific sites, to overcome the limitation of strong motion scarcity. The GP method has been used to successfully simulate broadband ground motions during the 1933 Long Beach earthquake (Hough and Graves, 2020), the 1906 San Francisco earthquake (Aagaard et al., 2008), the 1989 Loma Prieta earthquake (Graves and Pitarka, 2010), the 2011 Christchurch earthquake (Razafindrakoto et al., 2018), the 2019 Ridgecrest earthquake (Pitarka et al., 2021), and in other scenarios (Graves et al., 2008). In this study, synthetic broadband strong ground motions were simulated using the GP method. We used this method to simulate ground motions at specific sites and compute the spatial distribution of ground motion intensity measurements (PGA, peak ground acceleration; PGV, peak ground velocity; and SAs, acceleration response spectra) in the region where strong earthquake ground motion recordings were not available. These broadband simulations of strong ground motions have important applications in further analysis of earthquake damage to engineering structures near faults and for evaluating the performance of engineering structures. In addition, this study provides a basis for the future implementation of probabilistic seismic hazard analysis (PSHA) and seismic design on the Tibetan Plateau.
The hybrid broadband ground motion simulation methodology of Graves and Pitarka (2004, 2010) was used to compute ground motions for the 2021 M7.4 Maduo earthquake. This method combines a deterministic finite-difference calculation for frequencies f < 1.0 Hz with a stochastic calculation for frequencies 1.0 Hz < f < 20.0 Hz. The stochastic approach follows a semi-empirical ray-based theory that contains a stochastic source radiation pattern and simplified wave propagation through a 1D-layered approximate velocity model.
The low-frequency simulation methodology uses a theoretical rigorous representation of the source and wave propagation effects, derived from the elastic dynamics equation. It incorporates both complex source rupture and wave propagation effects within an arbitrarily heterogeneous three-dimensional (3D) geologic structure. The basic calculation was carried out using a (3D) viscoelastic finite-difference algorithm (Graves, 1996; Day and Bradley, 2001), which was solved by implementing a staggered-grid finite-difference method to obtain fourth-order spatial and second-order temporal accuracies. Applications of this finite-difference methodology have been described by Graves (1996) and Pitarka (1999).
The moment tensor components are represented as an equivalent distribution of body-force couples that are added to the individual components of velocity (here, the body forces in the xx and xy components are listed):
fxi+1/2,j,k=Mxx(t)h4,fxi−1/2,j,k=−Mxx(t)h4, |
fxi−1/2,j+1,k=Mxy(t)4h4,fxi+1/2,j+1,k=Mxy(t)4h4, | (1) |
fxi−1/2,j−1,k=−Mxy(t)4h4,fxi+1/2,j−1,k=−Mxy(t)4h4, |
where Mxx and Mxy are Cartesian moment tensor components acting in the x direction using equivalent body-force components, and h is the length of the moment arm.
The representation of the source rupture via sub-fault moment tensors depends on the numerical scheme adopted. In the GP method, the body forces (moment tensor) are the summation of the finite earthquake sources, which is specified by an explicit kinematic description of fault rupture, incorporating spatial heterogeneity in slip, rupture velocity, and rise time, or the source time function of each sub-fault. The low-frequency simulation dictates a grid size of 0.1 km for the fourth-order finite-difference operators to obtain results with frequencies up to 1 Hz.
Anelastic attenuation was also incorporated into the simulation of wave propagation within the 3D subsurface geological structure (Graves, 1996):
A=exp(−πf0tQ), | (2) |
where f0 is the corner frequency, Q is the quality factor, and t denotes the travel time.
In the GP method, the fault is discretized into i=1toN sub-faults with prescribed slip δi. Seismic waves travel from the source along the j=1toM ray path (e.g., direct and Moho-reflected). We summed the responses of the sub-faults by assuming a random phase, a wave number squared source spectrum and simplified Green′s functions calculated from a specified 1D velocity structure.
To construct the Fourier amplitude spectrum for a given site, the source and path components for a finite fault were summed as follows:
A(f)=N∑i=1M∑j=1CijSi(f)Gij(f)P(f). | (3) |
The source spectrum accounting for the radiation of sub-fault i and ray path j includes a frequency-independent term Cij and a frequency-dependent seismic radiation spectrum Si(f). The radiation pattern, shear wave velocity, and mass density at the center of the sub-fault were incorporated in Cij. Si(f) involves a shaping factor that scales the sub-fault corner frequency to that of the mainshock to ensure that the total moment of the sub-faults is the same as the mainshock moment. The source acceleration spectrum CijSi(f) is broadband with an ascending branch that scales with the square of the frequency and a flat branch for frequencies beyond the corner frequency fci.
The path Green′s function is given by
Gij(f)=Ii(f)Rijexp[−πfLj∑k=1ΔtkjQk(f)], | (4) |
where Rij represents the ray path distance from the sub-fault i to the site along the path. Iij(f) represents gross impedance effects calculated following quarter wavelength theory that uses a velocity model specified k=1toLj layers with thickness Δzk, shear wave velocity Vsk, and the whole path attenuation term Qk. The term Δtkj represents the travel time of a given ray through layer k.
In Equation (3), P(f) models high-frequency decay using the empirical κ0 parameter:
P(f)=e−πκ0f. | (5) |
The source rupture model used in this paper was proposed by Wang WM et al. (2022) and was generated from joint inversion of seismic waveforms and InSAR coseismic displacement data. This study utilizes the source finite-fault model based on 7 fault planes with a width of 28 km and a dip of 84°, following Wang WM et al. (2022), as shown in Figure 2. Rupture propagated in both directions along the fault plane and produced 7 surface ruptures, which reached a total length of 186 km. The slip distribution of the Maduo earthquake presents three high-slip zones in the eastern, middle, and western parts of the fault plane. During the eastern propagation of the source rupture, a peak slip value of 682 cm occurred near 99°E, and the strike at the eastern end of the fault was deflected toward the north. During the western propagation of the source rupture, a peak slip value of 357 cm occurred near 97.8°E, and the strike at the western end of the fault was deflected towards the south (Wang WM et al., 2022). The detailed source fault parameters obtained by Wang WM et al. (2022) include the seismic moment of 2.27×1020 N·m, which corresponds to a moment magnitude of 7.51, fault geometry (e.g., length, width, strike and dip), and rupture initiation point (hypocenter), as shown in Table 1.
Fault segment | Strike (°) | Dip (°) | Length (km) | Width (km) | Subfault size (km × km) |
1 | 263.00 | 84 | 36 | 28 | 6×4 |
2 | 287.00 | 84 | 18 | 28 | 6×4 |
3 | 278.50 | 84 | 18 | 28 | 6×4 |
4 | 285.50 | 84 | 48 | 28 | 6×4 |
5 | 271.50 | 84 | 6 | 28 | 6×4 |
6 | 294.00 | 84 | 18 | 28 | 6×4 |
7 | 277.00 | 84 | 42 | 28 | 6×4 |
Note: The dimension of subfaults is the result of inversion set by Wang WM et al. (2022). |
Subsequently, to simulate the ground motion of the 2021 M7.4 Maduo earthquake, we utilized the Wang source rupture model from inversions instead of using the kinematic rupture model generated by the stochastic slip generator of Graves and Pitarka (2016). The Wang rupture model represents the overall rupture process of the earthquake, containing entire spatiotemporal evolutions of the rupture, such as the fault geometry, subfault size, rupture velocity, as well as the rise time, moment, and source time functions of each subfault.
To incorporate the influence of the propagation path on the simulation results, we adopted the actual velocity model of the epicentral region of the M7.4 Maduo earthquake, which includes the influence of earth structure on ground motions. Xia SR et al. (2021) used the double-difference tomography method to image the 3D P- and S-wave velocity structures of the crust and upper mantle around the northeastern margin of the Tibetan Plateau. To simplify the calculation, we simplified the 3D velocity structure of the crust and upper mantle beneath the northeastern margin of the Tibetan Plateau into a 1D velocity model by averaging the P-wave velocity, S-wave velocity, and medium density at different depths, as shown in Figure 3.
During the Maduo earthquake, 16 strong-motion stations were triggered and recorded ground motions; 7 of these recordings were incomplete. Most of these observation stations are situated in the far-field region, more than 180 km from the epicenter, and these recordings have no engineering significance. Only stations 63DAW and 63XIH are located in the regional simulation domain illustrated in Figure 1, at distances of 175.47 km and 186.97 km from the epicenter, respectively. Nevertheless, the waveforms of all 16 distant stations illustrated in Figure 4 were simulated and validated against the observations. The epicentral distances of these stations are listed in Table 2.
Recorded stations | Epicentral distance (km) | Completeness of recordings |
63DAW | 175.47 | complete |
63XIH | 186.97 | complete |
63DUL | 191.37 | complete |
63TGM | 229.51 | complete |
63NMH | 266.04 | complete |
63GOH | 278.63 | incomplete |
63HEN | 300.52 | complete |
63DGL | 311.79 | complete |
63GUD | 321.32 | complete |
63DLH | 322.00 | complete |
63TOR | 342.63 | incomplete |
63HUY | 345.48 | incomplete |
63XIN | 381.31 | incomplete |
63PIA | 401.06 | incomplete |
63XUH | 402.71 | incomplete |
63MIH | 448.27 | incomplete |
The validation was conducted using the 16 strong motions available within 450 km of the epicenter. To prevent baseline drift and avoid loss of frequency information, the recordings were processed using the automatic baseline correction method proposed by Wang RJ et al. (2011). Figure 5 provides comparisons of the observed and simulated three-component acceleration broadband waveforms and their corresponding amplitudes at the 16 stations. Figure 6 provides comparisons of the observed and simulated three-component velocity broadband waveforms and amplitudes at the 16 stations. We found that the simulated amplitudes and durations of the three-component waveforms matched the recorded amplitudes and durations reasonably well at stations 63DAW and 63XIH. It should be noted that the PGA and PGV recorded at the other 14 stations were less than 10 cm/s2 and 5 cm/s, respectively. Although the simulated amplitudes are close to the recorded amplitudes, the effect of noise cannot be ignored. We noticed that recordings from 7 of the stations were incomplete. Comparisons of the duration time of shaking at the stations with missing partial recordings were not taken into account. Overall, a comparison of the waveforms reveals that the simulated waveforms are reasonably similar to the observed waveforms, in terms of amplitude and frequency. In general, the agreement between the simulated and observed waveforms is acceptable.
The SAs obtained from the recorded and simulated waveforms of station 63DAW were compared with the predictions from the NGA-West2 models, including the ASK2014 (Abrahamson et al., 2014), BSSA2014 (Boore et al., 2014), CB2014 (Campbell and Bozorgnia, 2014), and CY2014 (Chiou and Youngs, 2014) models. Figure 7 indicates that the simulated results are within one standard deviation of the predictions from the ground motion prediction equations (GMPEs), during the period of 0–10 s. The response spectra from simulated ground motions, the response spectra from recorded ground motions, and predicted response spectra at 63DAW are in good agreement. Horizontal and vertical recorded and simulated SA of another eight complete recording stations are plotted in Figure 8. The values of the acceleration response spectra of these stations were approximately an order of magnitude smaller than those of 63DAW.
Figure 9 provides a comparison of the observed and simulated three-component Fourier amplitude spectra at stations 63DAW, 63XIH, 63DUL, and 63DLH. Both the level and trend of the observations were quite well matched by the simulations. Comparisons of the recorded and simulated three-component Fourier amplitude spectra at stations 63TGM, 63 NMH, 63HEN, 63DGL, and 63GUD are shown in Figure S1. In the high-frequency domain (greater than 1 Hz), the simulated Fourier amplitude spectra at most stations fit well with the recordings. We found that the simulation results underestimated the recorded values at 0.1–1 Hz at stations 63XIH and 63DUL. The absolute residuals of the Fourier amplitude spectra are small, showing little bias. The slight differences between the recorded and simulated Fourier amplitude spectra indicate that overall, the simulation could sufficiently reproduce the main characteristics of the ground motions observed during the Maduo earthquake.
Strong ground motions were simulated in a regular 0.2°×0.2° grid covering the study area (96°E–101°E, 33°N–36°N). To capture the variation in near-field ground motions, we employed a refined 0.1°×0.1° grid immediately surrounding the fault (97°E–99.5°E, 34°N–35.3°N). The study area was divided into 38×22 latitudinal and longitudinal grids. In short, this process generated 897 intersections and endpoints, which were defined as sites for our simulation. The rupture fault, macroseismic intensity distribution, and strong ground motion stations in the study area are shown in Figure 1.
To evaluate the applicability of the NGA-West2 models to the simulated results, we compared the simulated results with predictions from the NGA-West2 models. Figure 10 shows the variations in three intensity measures (IMs), namely, the PGA, PGV, and SA at various periods (T = 0.1, 0.3, 0.5, 1.0, 3.0, and 5.0 s) for the simulated ground motions with the rupture distance (Rrup). These IMs are also compared with the values predicted by the NGA-West2 models. Based on the simulated results, we also developed a simplified ground motion model that includes both geometric and anelastic attenuation terms with rupture distance Rrup, as shown in Figure 10. The functional form, similar to the Campbell and Bozorgnia (2014) model, is given as
lnY=a+b×ln√R2rup+c2+d×Rrup+σlnY, | (6) |
where Y represents the intensity measures; a, b, c, and d are coefficients derived from least-squares regression analysis; and σlnY is the standard deviation of the regression.
As shown in Figure 10a, c, d, e, and f, for PGA and SA values at short periods (T = 0.1, 0.3, 0.5, and 1.0 s), the median IM values fitted by simulations are slightly smaller than the median predictions from the four NGA-West2 models when Rrup ≤ 10 km. Nevertheless, when Rrup > 10 km, the median IM values fitted by simulations are more consistent with the median predictions. Overall, most of the simulated results fall within one standard deviation to either side of the values predicted by the four NGA-West2 models. However, Figure 10b, g, and h suggest that at longer periods (T = 3.0 s and 5.0 s), the fitted median simulated PGV and SA values are underestimated relative to the four NGA-West2 models over the whole distance range. The results suggest that the NGA-West2 models may not be suitable for describing ground motions for the long periods of the Maduo event, which occurred in the high-altitude hinterland of the eastern Tibetan Plateau.
Coefficients | R2 | σ | ||||
a | b | c | d | |||
PGA | 7.3130 | −0.6644 | 9.608 | −0.007 | 0.9276 | 0.2432 |
PGV | 5.5020 | −0.08627 | 8.32 | 0 | 0.8999 | 0.2171 |
SA (0.1 s) | 8.2420 | −0.7850 | 10.028 | −0.0074 | 0.9353 | 0.2556 |
SA (0.3 s) | 8.0130 | −0.6026 | 9.201 | −0.007 | 0.9151 | 0.2627 |
SA (0.5 s) | 7.9870 | −0.6223 | 9.193 | −0.0062 | 0.8941 | 0.2731 |
SA (1.0 s) | 7.6060 | −0.6322 | 9.739 | −0.0047 | 0.8748 | 0.2716 |
SA (3.0 s) | 4.6060 | −0.4655 | 4.68 | −0.0014 | 0.6627 | 0.3254 |
SA (5.0 s) | 4.3660 | −0.4987 | 4.199 | 0 | 0.6967 | 0.2851 |
Note: R2 is a determination coefficient; σ signifies 1 standard deviation of the regression. |
We investigated the spatial variation of the simulated PGA, PGV, and pseudo-spectral acceleration (PSA) at various periods (T = 0.1, 0.3, 0.5, 1.0, 3.0, and 5.0 s), as shown in Figures 11–13. The contours in these figures are elongated along the fault trace. Our simulations indicate that shaking intensity was significantly higher along the strike of the rupture and lower in the direction normal to the rupture, showing the significant rupture directivity effect. As can be seen from Figure 11, there are four concentrated areas with high PGA values in the gradient contour map. The location where the maximum PGA value reaches 575.26 cm/s2 is near the intersection of fault zones 6 and 7, rather than near the epicenter. Two regions with concentrated high PGV values can also be seen in Figure 12, near the intersection of fault segments 2 and 3 and the intersection of fault segments 5 and 6, with the maximum PGV reaching 45.42 cm/s. Figure 13 plots PSA distributions at various periods; the acceleration spectra corresponding to 0.1 s, 0.3 s, and 0.5 s are larger than those corresponding to 1.0 s, 3.0 s, and 5.0 s. Simulated PSA shows a relatively rapid attenuation with the period and weak dependence on the fault dimension. This indicates the high-frequency components of ground motions generated for the 2021 Maduo M7.4 earthquake using the GP method are more prominent than the low-frequency components. This result may be related to the multi-rupture fault model. Moreover, the low-frequency (long-period) PSA contours enclose a larger affected area than the high-frequency contours, extending from the near to middle-far field. Cao ZL et al. (2021) obtained similar results in the simulation of three-component ground motions of the Maduo earthquake. Nevertheless, we can infer from the simulation (Figure 11 to Figure 13) that the high-frequency ground motions are severely influenced by the details of the source rupture model, especially in the near-field region.
As mentioned previously, the shakemap of macroseismic intensity distribution for the Maduo earthquake is only an approximation, as it has very low resolution and large uncertainty in sparsely populated and high-altitude regions. Thus, the seismic intensity distributions were simulated and compared with the macroseismic intensities to overcome these shortcomings. We computed the seismic intensity from our simulations using the relationships between peak horizontal velocity, PGA, and modified Mercalli intensity (MMI) developed for shake maps (Wald et al., 1999, 2005). The functional form is given by Aagaard et al. (2008) as
MMI={MMIPGA,ifMMI<V12[(VII−MMIPGA)×MMIPGA+(MMIPGA−V)×MMIPGV],ifV≤MMI≤VIIMMIPGV,ifMMI≥VII, | (7) |
MMIPGA={2.20×logPGA+1.00,ifMMI<V3.66×logPGA−1.66,ifMMI≥V, | (8) |
MMIPGV={2.10×logPGA+3.40,ifMMI<V3.47×logPGA+2.35,ifMMI≥V, | (9) |
Figure 14a displays the macroseismic intensity map issued by the Ministry of Emergency Management of the People′s Republic of China. Figure 14b displays a synthetic intensity map from simulations of the Maduo earthquake created with the Wang source model. The synthetic seismic intensities reveal a distribution of ground motion intensity with two regions of concentrated high values. Simulated seismic intensities were highest along the fault, especially where the estimated slip was high, and decreased rapidly along the direction perpendicular to strike. Figure 14c shows the intensity residuals between the synthetic intensity distribution and the reference macroseismic intensity distribution. These differences remain obvious. The misfit is largest in the far-field, where the evaluated intensities are at most two MMI units higher than the simulated intensities over significant areas. In most sites, the simulated intensity is 1 unit lower than the macroseismic intensity. Figure 14d shows a histogram of the difference between simulated and macroseismic intensities that approximately obeys the normal distribution and reveals a macroseismic intensity overestimation of one unit, with a mean residual of −0.87 and standard deviation of 0.53.
We generated a map of intensity distribution within this region for the Maduo earthquake, based on multiple constraints including a detailed rupture model, regional velocity model with high resolution, and GP broadband simulation method. Thus, we assume that this map is more accurate than the macroseismic intensity map released by the Ministry of Emergency Management of the People′s Republic of China, with its low resolution and large uncertainties in high-altitude regions. A comparison of the two maps indicates that the latter tends to overestimate the ground shaking caused by the Maduo earthquake. The presented simulations provide ground motions that can be used to analyze the seismic performance of engineering structures in the 2021 Maduo earthquake.
It would be useful if ground motions could be deliberately simulated at selected sites that were lacking in ground motion records. In the Maduo region where ground motion recordings are sparse or non-existent, ground motion time histories are necessary for analyzing the structural seismic responses to this earthquake. The such analysis aids in estimating building damage and evaluating the performance of engineering structures at major damage sites. The 9 sites indicated in green in Figure 1 were chosen as a representative sample spanning the region covered by the simulation. Details of the locations of these sites are listed in Table 4. Figure 15 illustrates the three components of the simulated acceleration time histories, velocity time histories, and response spectra at the nine selected sites. The spatial variability of PGA and PGV at the selected sites was inspected. The sites A01, A02, A03, A04, and A05 near the faults were found to show larger amplitudes, whereas the sites A06, A07, A08, and A09 at a larger distance from the faults show lower-amplitude ground motions.
Site | Longitude (°E) | Latitude (°N) | Intensity |
A01 | 98.00 | 34.70 | X |
A02 | 98.10 | 34.70 | IX |
A03 | 98.50 | 34.50 | VIII |
A04 | 97.70 | 34.80 | VIII |
A05 | 99.00 | 34.40 | IX |
A06 | 98.20 | 34.30 | VII |
A07 | 96.70 | 35.10 | VI |
A08 | 98.10 | 35.30 | VI |
A09 | 99.50 | 33.40 | V |
Note: The "Intensity" means the site locates in the corresponding intensity region which was released by the Ministry of Emergency Management of China in Figure 1. |
These simulations can be directly used as ground motion inputs for dynamic analysis of forensic structural and geotechnical responses. During the earthquake, the Yematan Bridge (34.68°N, 98.06°E) and Yematan No. 2 Bridge (34.65°N, 98.04°E) on the Gongyu section of the Xili Expressway collapsed due to falling beams. The two bridges, located approximately 27 km from the epicenter between sites A01 and A02, experienced similar amplitudes and waveforms in the horizontal and vertical components. Based on these simulated results, we can infer that the Yematan Bridge and Yematan No. 2 Bridge suffered a peak acceleration of approximately 400 cm/s2 at ground level during the earthquake. Simulated time histories at the A01 and A02 sites can be used to analyze the damage to the two bridges and understand their seismic performance.
We restricted our broadband ground motion simulations to simplified wave propagation through a 1D-layered approximation of a 3D velocity model. The 1D layered region-specific velocity structure model was obtained from the local regional dataset and was used to calculate Green′s function, anelastic attenuation, and ground motion simulations for this earthquake. We recognize that the effects of surface topography were not considered, and our simulations do not take into account the effects of heterogenous 3D wave propagation, which modulate the resulting ground shaking levels and their distributions. Unfortunately, detailed 3D crustal models are limited to a few small areas worldwide and commonly suffer from limited spatial resolution (Imperatori and Mai, 2012). Modeling of complex wave propagation phenomena associated with the 3D structure of this region may require further explicit inclusion of surface topography effects in the numerical simulation GP method for regional ground motion simulation.
Combining the kinematic source model of the 2021 Maduo M7.4 earthquake from Wang WM et al. (2022) with a high-resolution regional seismic velocity model allowed for the successful simulation of primary spatial variations in shaking intensity. The simulated data showed good agreement with the data recorded at station 63DAW, indicating that simulations of this event could be used to study the ground motion characteristics in the near-fault region. The waveforms, acceleration response spectra, and Fourier amplitude spectra at triggered strong motion stations were used to validate the observations. The simulations provided a reasonable fit for the observations. In general, the agreement between observations and simulations is acceptable. Ground motions were simulated at 897 virtual grid stations in the epicentral region and presented as PGA, PGV, and SA contour plots. In addition, the acceleration and velocity time histories and response spectra were provided for the selected representative sites where no strong motion recordings were available. Our results indicate that the officially released macroseismic intensities for the 2021 Maduo earthquake have large uncertainties in sparsely populated high-altitude regions and the ground shakings are generally overestimated by an average of one MMI unit in most sites of the epicenter region. The spatial distributions of PGA, PGV, SA, and MMI in the near-field region reveal two relatively high-value concentrations that correspond to the surface projection of the high-slip area on the fault plane, indicating the dominant effect of the source rupture model in the near-field simulation. Moreover, the results suggest uneven distributions of PGA, PGV, and SA, reflecting the complexity of the source rupture model. Our simulations show that the high-frequency components of ground motions were prominent, while the low-frequency components were not. This phenomenon is unexpected for large earthquakes and may be related to the multi-segment fault rupture caused by this large earthquake. Our research suggests that the four NGA-West2 models are effective at describing ground motions for short periods. However, NGA-West2 models are not suitable for describing ground motions for the long periods of the Maduo event, which occurred in the high-altitude hinterland of the eastern Tibetan Plateau.
We conclude that in light of recent knowledge of the source rupture model, regional and local velocity structure, and hybrid broadband ground motion simulation techniques, our simulation of the 2021 Maduo earthquake ground motions has yielded reliable and useful results. Hence, the simulated results have important implications for evaluating the performance of engineering structures in the epicentral regions of this earthquake and for estimating seismic hazards in the Tibetan regions where no strong ground motion records of large earthquakes are available. Similarly, these simulated results can provide data support for refining macroseismic intensity maps in sparsely populated areas with few buildings.
The authors thank the National Strong-Motion Observation Network System (NSMONS) of China for providing the strong motion data for the Maduo M7.4 earthquake. We appreciate the detailed explanation of the source rupture process provided by Prof. Weimin Wang. We would like to thank Prof. Yonghua Li and Dr. Lei Shi for providing the digital 3D model of the velocity structure of the crust and upper mantle beneath the northeastern margin of the Tibetan Plateau. The authors thank Graves and Pitarka for making their code, relating to broadband ground motion simulation, available online. The authors also thank Prof. Yongge Wan for his help. The constructive reviews provided by all anonymous reviewers were very helpful in revising the paper. Financial support for this study was provided by the National Key Research and Development Project (No. 2020YFA0710603) and the Special Fund of the Institute Geophysics, China Earthquake Administration (No. DQJB22B27).
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Fault segment | Strike (°) | Dip (°) | Length (km) | Width (km) | Subfault size (km × km) |
1 | 263.00 | 84 | 36 | 28 | 6×4 |
2 | 287.00 | 84 | 18 | 28 | 6×4 |
3 | 278.50 | 84 | 18 | 28 | 6×4 |
4 | 285.50 | 84 | 48 | 28 | 6×4 |
5 | 271.50 | 84 | 6 | 28 | 6×4 |
6 | 294.00 | 84 | 18 | 28 | 6×4 |
7 | 277.00 | 84 | 42 | 28 | 6×4 |
Note: The dimension of subfaults is the result of inversion set by Wang WM et al. (2022). |
Recorded stations | Epicentral distance (km) | Completeness of recordings |
63DAW | 175.47 | complete |
63XIH | 186.97 | complete |
63DUL | 191.37 | complete |
63TGM | 229.51 | complete |
63NMH | 266.04 | complete |
63GOH | 278.63 | incomplete |
63HEN | 300.52 | complete |
63DGL | 311.79 | complete |
63GUD | 321.32 | complete |
63DLH | 322.00 | complete |
63TOR | 342.63 | incomplete |
63HUY | 345.48 | incomplete |
63XIN | 381.31 | incomplete |
63PIA | 401.06 | incomplete |
63XUH | 402.71 | incomplete |
63MIH | 448.27 | incomplete |
Coefficients | R2 | σ | ||||
a | b | c | d | |||
PGA | 7.3130 | −0.6644 | 9.608 | −0.007 | 0.9276 | 0.2432 |
PGV | 5.5020 | −0.08627 | 8.32 | 0 | 0.8999 | 0.2171 |
SA (0.1 s) | 8.2420 | −0.7850 | 10.028 | −0.0074 | 0.9353 | 0.2556 |
SA (0.3 s) | 8.0130 | −0.6026 | 9.201 | −0.007 | 0.9151 | 0.2627 |
SA (0.5 s) | 7.9870 | −0.6223 | 9.193 | −0.0062 | 0.8941 | 0.2731 |
SA (1.0 s) | 7.6060 | −0.6322 | 9.739 | −0.0047 | 0.8748 | 0.2716 |
SA (3.0 s) | 4.6060 | −0.4655 | 4.68 | −0.0014 | 0.6627 | 0.3254 |
SA (5.0 s) | 4.3660 | −0.4987 | 4.199 | 0 | 0.6967 | 0.2851 |
Note: R2 is a determination coefficient; σ signifies 1 standard deviation of the regression. |
Site | Longitude (°E) | Latitude (°N) | Intensity |
A01 | 98.00 | 34.70 | X |
A02 | 98.10 | 34.70 | IX |
A03 | 98.50 | 34.50 | VIII |
A04 | 97.70 | 34.80 | VIII |
A05 | 99.00 | 34.40 | IX |
A06 | 98.20 | 34.30 | VII |
A07 | 96.70 | 35.10 | VI |
A08 | 98.10 | 35.30 | VI |
A09 | 99.50 | 33.40 | V |
Note: The "Intensity" means the site locates in the corresponding intensity region which was released by the Ministry of Emergency Management of China in Figure 1. |