Statistical Methods and Modeling of Seismogenesis. Eleftheria Papadimitriou

Statistical Methods and Modeling of Seismogenesis - Eleftheria Papadimitriou


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are represented in Figure 1.4, taken from Lasocki and Papadimitriou (2006). We can see that the kernel estimate better fits the observed data, though the difference between these two estimates in the larger magnitude range is pretty tiny. However, due to the significant impact of the magnitude CDF on the parameters of hazard [1.17] and [1.18], the difference between the mean return period estimates is dramatic. For instance, for magnitude 6.5, the return period obtained from the exponential distribution model is close to 100 years. The kernel estimate of this return period is less than 10 years. Lasocki and Papadimitriou (2006) compared the “exponential” and “kernel” estimates of the mean return period for different magnitudes, with the estimates drawn from the actual observations done in the preceding 94 years (Figure 1.5). The differences between the “kernel” estimates and the assessments from actual observations were insignificant compared to the huge deviation of the “exponential” estimate. This led to the conclusion that the “kernel” estimate was much better than the “exponential” one.

      Also, many other studies indicated big differences between the “exponential” and “kernel” estimates of hazard parameters. The mentioned Monte Carlo analyses by Kijko et al. (2001), and the actual data studies by Lasocki and Papadimitriou (2006), suggest that in the case when these estimates differ, the “kernel” estimate is more accurate. All of this favors the kernel estimation of magnitude distribution functions for the seismic hazard assessment.

      The PSHA, which uses the kernel estimation of magnitude distribution as an alternative to the parametric model [1.19] and [1.20], has been implemented on the IS-EPOS Platform (tcs.ah-epos.eu, Orlecka-Sikora et al. 2020). The kernel estimation of magnitude distribution is also applied in the SHAPE software package for time-dependent seismic hazard analysis (Leptokaropoulos and Lasocki 2020). SHAPE is open-source, downloadable from https://git.plgrid.pl/projects/EA/repos/seraapplications/browse/SHAPE_Package.

      Orlecka-Sikora (2004, 2008) presented a method for assessing the confidence intervals of the CDF, which had been estimated by the kernel estimation. The method is based on the bias-corrected and accelerating method by Efron (1987), the smoothed bootstrap and the second-order bootstrap samples, and is called the iterative bias-corrected and accelerating method (IBCa).

      The j-th jackknife sample, jn, is the n − 1 element sample {M1, M2,.., Mj−1, Mj+1, .., Mn} that is the initial sample from which the j-th element has been removed. Hence, we can have, at most, n jackknife samples.

      The first-order smoothed bootstrap samples are obtained in the same way as previously (equation [1.25]). The k-th smoothed bootstrap sample, (k), is composed of:

      [1.33]image

      [1.34]image

      where is the standard bootstrap sample from (k).

      The IBCa method can be presented in the following steps:

       – Step 1. Generate n jackknife samples, estimate kernel CDF-s from the jackknife samples, and evaluate the accelerating constant:

      [1.35]image

      where stands for the arithmetic mean of

       –


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