Statistical Methods and Modeling of Seismogenesis. Eleftheria Papadimitriou

Statistical Methods and Modeling of Seismogenesis - Eleftheria Papadimitriou


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2.12. Map of ruptures for M ≥ 6.0 earthquakes on the joint set of three faults of the 24 adopted in the model, in 33 time windows of 300 years represented from top to bottom. The 170 km long fault system is displayed in each panel from left to right moving from NW to SE (Figure 1 of Console et al. (2018a)). On any panel, the level of darkness represents the temporal order of earthquake occurrence, and the amount of slip on multiply ruptured cells (based on Console et al. (2018a))

      By examining Figure 2.12, we note that only three 300 years periods of 33 were lacking any M ≥ 6.0 earthquake, while only two of the other periods contain three earthquakes of such magnitude. There is a clear trend for earthquakes not to occupy the same rupture areas in the same time window, or in consecutive time windows, while they are mostly separated from each other by more than 300 years of several time windows. During the whole test of 10,000 years, every portion of the 170 km long fault system was occupied by at least six or seven ruptures in distinct earthquakes, and none of them was left empty. This is consistent with the recurrence time of 500–1,000 years characterizing the three faults considered in this test.

      From the results of this exercise (see Figure 2.12), we can infer that the segmentation scheme mainly based on historical records of earthquakes occurred during the latest centuries could have likely been conditioned by the particular pattern of ruptures exhibited by a group of sources in this relatively recent time window.

      2.3.6. Further improvements of the simulator code (2019)

      In the last version of the simulator, we introduced new features with the aim of achieving a more realistic physical modeling of the seismic process and a better similarity between real and synthetic catalogs. The first improvement in the new version of the algorithm is the modeling of the geometry of the seismic source by a trapezoidal shape, of which the old rectangles are a limit case. The rationale of this change is to allow a more accurate modeling of curve seismogenic structures, as described in the previous section, avoiding gaps between adjacent rectangular faults with different strikes. In the numerical application, the discretization of the trapezoidal shapes of the faults in square cells is obtained by retaining only the cells the centers of which are inside the trapeze edges. Note that modeling the seismic sources by numerous faults of rectangular or trapezoidal shape is just a convenient tool for the simplicity of the algorithm used in the physics-based simulator code, but in no way does it constitute a limitation to stop a rupture at the edges of such faults.

      where γ0 and r0 are the unperturbed steady-state values of γ and r. Here r0 is the rate of events of magnitude exceeding the threshold adopted in the simulation. It is obtained by dividing the slip rate of each fault segment in the seismogenic model by the slip pertaining to an event of average magnitude, assuming a G-R magnitude distribution with b = 1, for events of magnitude exceeding the threshold. Every cell changes its stress status and consequently the values of γ and r when an event occurs not very far in the fault system. The coseismic Coulomb stress change ΔCFF on the receiving cell is computed by:

      [2.4]image

Schematic illustration of computer code for earthquake simulation with rate- and-state constitutive law nucleation mechanism.
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