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Physics-based probabilistic seismic hazard analysis: the case of Tehran Basin in Iran

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Abstract

Seismic hazard estimation relies on Ground Motion Prediction Equations (GMPEs) giving the expected motion level as a function of several parameters characterizing the source and the sites of interest. However, in regions like Greater Tehran metropolitan area located in the Alborz seismotectonic province, northern Iran records of moderate to large earthquakes at short distances from the faults are still few and most local and regional GMPEs are poorly constrained at short ranges. In other words, data may only partially account for the rupture process, seismic wave propagation, and three-dimensional complex configurations (i.e., Tehran Basin in this case). Here, to investigate the capabilities of physics-based methods, two sets of 3-D numerical simulations of possible earthquakes scenarios in Tehran region along two predominate sources are carried out through the finite difference approach for low frequency motions. Then the stochastic finite fault method is used for quantifying ground motion values at higher frequencies. At last, the combined broadband simulation results are used in a probabilistic seismic hazard analysis. The seismic hazard results show the combined effects of the site and basin, and give a high-resolution representation of the hazard in the near field of active earthquake faults in the Tehran Basin, particularly over long periods. This representation is anticipated to be more accurate than those based simply on empirical GMPEs. It should be noted that effects of other less important surrounding faults are not included in the hazard analysis due to lack of sufficient data and computational limitations.

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Data availability

The data generated during the current study are available from the corresponding author on reasonable request.

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Acknowledgements

We would like to sincerely thank Dr. Anooshiravan Ansari and Dr. Leila EtemadSaeed for their support. The authors would like to acknowledge Iran National Science Foundation (INSF) for its support. This work was supported by INSF under Grant No [4002707]. This study was supported by the International Institute of Earthquake Engineering and Seismology (IIEES), and is a part of project: “Physics Based Probabilistic Seismic Hazard Analysis by considering uncertainties, case study: Tehran region”.

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RA: Material preparation, Data collection and analysis, Simulation, Writing the manuscript. HZ: Discussed the results, commented on the manuscript and supervision.

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Correspondence to Hamid Zafarani.

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Appendices

Appendix 1: Sensitivity of numerical simulations to hypocenter location, slip distribution and stress drop. Note that ratio maps are in natural logarithm

Section 1 North Tehran Fault.

See Figs.

Fig. 26
figure 26

PGV ratio maps between numerical simulations for different hypocenters and GMPEs: simulation with hypocenter 1(up left) simulation with hypocenter 2(up right), simulation with hypocenter 3(down left), All simulation (down right)

26,

Fig. 27
figure 27

PGV ratio maps between numerical simulations for different slip distributions and GMPEs: simulation with slip distribution 1(up left) simulation with slip distribution 2(up right), simulation with slip distribution 3(middle left), simulation with slip distribution 4(middle right), simulation with slip distribution 5(down left), All simulation (down right)

27,

Fig. 28
figure 28

PGV ratio maps between numerical simulations for different stress drops and GMPEs: simulation with stress drop 1(up left) simulation with stress drop 2(up right), simulation with stress drop 3(down left), All simulation (down right)

28.

Section 2 Kahrizak Fault.

See Figs.

Fig. 29
figure 29

PGV ratio maps between numerical simulations for different hypocenters and GMPEs: simulation with hypocenter 1(up left) simulation with hypocenter 2(up right), simulation with hypocenter 3(down left), All simulation (down right)

29,

Fig. 30
figure 30

PGV ratio maps between numerical simulations for different slip distributions and GMPEs: simulation with slip distribution 1(up left) simulation with slip distribution 2(up right), simulation with slip distribution 3(middle left), simulation with slip distribution 4(middle right), simulation with slip distribution 5(down left), All

30,

Fig. 31
figure 31

PGV ratio maps between numerical simulations for different stress drops and GMPEs: simulation with stress drop 1(up left) simulation with stress drop 2(up right), simulation with stress drop 3(down left), All simulation (down right)

31.

Appendix 2: Statistical analysis of the numerical simulations

Section 1 North Tehran Fault.

See Figs.

Fig. 32
figure 32

Comparison between the normalized residuals from the 3D simulations (blue curves) and the theoretical normal distribution for receiver 5 at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s, in terms of probability density functions (top panels), cumulative density functions (central panels) and normal plots (bottom panels)

32,

Fig. 33
figure 33

Comparison between the normalized residuals from the 3D simulations (blue curves) and the theoretical normal distribution for receiver 63 at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s, in terms of probability density functions (top panels), cumulative density functions (central panels) and normal plots (bottom panels)

33,

Fig. 34
figure 34

Comparison between the normalized residuals from the 3D simulations (blue curves) and the theoretical normal distribution for receiver 97 at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s, in terms of probability density functions (top panels), cumulative density functions (central panels) and normal plots (bottom panels)

34,

Fig. 35
figure 35

Comparison between the spectral displacement at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s from the 3D simulations (blue curves) and the theoretical gamma distribution for receiver 5 in terms of probability density functions (top panels) and cumulative density functions (bottom panels)

35,

Fig. 36
figure 36

Comparison between the spectral displacement at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s from the 3D simulations (blue curves) and the theoretical gamma distribution for receiver 63 in terms of probability density functions (top panels) and cumulative density functions (bottom panels)

36,

Fig. 37
figure 37

Comparison between the spectral displacement at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s from the 3D simulations (blue curves) and the theoretical gamma distribution for receiver 97 in terms of probability density functions (top panels) and cumulative density functions (bottom panels)

37 and Tables

Table 5 Results of the X 2 test carried out for the three receivers and for two spectral ordinates (T = 1 s and T = 5 s)

5,

Table 6 Results of the Kolmogorov- Smirnoff test carried out for the three receivers and for two spectral ordinates (T = 1 s and T = 5 s)

6,

Table 7 Results of the Anderson–Darling test carried out for the three receivers and for two spectral ordinates (T = 1 s and T = 5 s)

7.

Section 2 Kahrizak Fault.

See Figs.

Fig. 38
figure 38

Comparison between the normalized residuals from the 3D simulations (blue curves) and the theoretical normal distribution for receiver 46 at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s, in terms of probability density functions (top panels), cumulative density functions (central panels) and normal plots (bottom panels)

38,

Fig. 39
figure 39

Comparison between the normalized residuals from the 3D simulations (blue curves) and the theoretical normal distribution for receiver 113 at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s, in terms of probability density functions (top panels), cumulative density functions (central panels) and normal plots (bottom panels)

39,

Fig. 40
figure 40

Comparison between the normalized residuals from the 3D simulations (blue curves) and the theoretical normal distribution for receiver 135 at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s, in terms of probability density functions (top panels), cumulative density functions (central panels) and normal plots (bottom panels)

40,

Fig. 41
figure 41

Comparison between the spectral displacement at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s from the 3D simulations (blue curves) and the theoretical gamma distribution for receiver 46 in terms of probability density functions (top panels) and cumulative density functions (bottom panels)

41,

Fig. 42
figure 42

Comparison between the spectral displacement at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s from the 3D simulations (blue curves) and the theoretical gamma distribution for receiver 113 in terms of probability density functions (top panels) and cumulative density functions (bottom panels)

42,

Fig. 43
figure 43

Comparison between the spectral displacement at 3 vibration periods T = 0.5 s, T = 1 s and T = 5 s from the 3D simulations (blue curves) and the theoretical gamma distribution for receiver 135 in terms of probability density functions (top panels) and cumulative density functions (bottom panels)

43 and Tables

Table 8 Results of the X 2 test carried out for the three receivers and for two spectral ordinates (T = 1 s and T = 5 s)

8,

Table 9 Results of the Kolmogorov- Smirnoff test carried out for the three receivers and for two spectral ordinates (T = 1 s and T = 5 s)

9,

Table 10 Results of the Anderson–Darling test carried out for the three receivers and for two spectral ordinates (T = 1 s and T = 5 s)

10.

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Alikhanzadeh, R., Zafarani, H. Physics-based probabilistic seismic hazard analysis: the case of Tehran Basin in Iran. Bull Earthquake Eng 21, 6171–6214 (2023). https://doi.org/10.1007/s10518-023-01785-w

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