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ORIGINAL PAPER Applicability of different ground-motion prediction models for northern Iran H. Zafarani M. Mousavi Received: 17 June 2013 / Accepted: 16 February 2014 Ó Springer Science+Business Media Dordrecht 2014 Abstract A total of 163 free-field acceleration time histories recorded at epicentral distances of up to 200 km from 32 earthquakes with moment magnitudes ranging from M w 4.9 to 7.4 have been used to investigate the predictive capabilities of the local, regional, and next generation attenuation (NGA) ground-motion prediction equations and determine their applicability for northern Iran. Two different statistical approaches, namely the likelihood method (LH) of Scherbaum et al. (Bull Seismol Soc Am 94:341–348, 2004) and the average log-likelihood method (LLH) of Scherbaum et al. (Bull Seismol Soc Am 99:3234–3247, 2009), have been applied for evaluation of these models. The best-fitting models (considering both the LH and LLH results) over the entire frequency range of interest are those of Ghasemi et al. (Seismol 13:499–515, 2009a) and Soghrat et al. (Geophys J Int 188:645–679, 2012) among the local models, Abrahamson and Silva (Earthq Spectra 24:67–97, 2008) and Chiou and Youngs (Earthq Spectra 24:173–215, 2008) among the NGA models, and finally Akkar and Bommer (Seism Res Lett 81:195–206, 2010) among the regional models. Keywords Ground-motion prediction equations Evaluation of fitness Ranking PSHA Northern Iran 1 Introduction The treatment of uncertainty is the greatest challenge in the current probabilistic seismic hazard analysis (PSHA) and is an active area of research. It is well known that uncertainty H. Zafarani (&) International Institute of Earthquake Engineering and Seismology (IIEES), No. 26, Arghavan St., North Dibajee, Farmanieh, P.O. Box 19395/3913, Tehran, Iran e-mail: [email protected]; [email protected] M. Mousavi Department of Civil Engineering, Faculty of Engineering, Arak University, Ara ¯k, Iran 123 Nat Hazards DOI 10.1007/s11069-014-1151-2

Applicability of different ground-motion prediction models for northern Iran

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  • ORI GIN AL PA PER

    Applicability of different ground-motion predictionmodels for northern Iran

    H. Zafarani M. Mousavi

    Received: 17 June 2013 / Accepted: 16 February 2014 Springer Science+Business Media Dordrecht 2014

    Abstract A total of 163 free-field acceleration time histories recorded at epicentraldistances of up to 200 km from 32 earthquakes with moment magnitudes ranging from Mw4.9 to 7.4 have been used to investigate the predictive capabilities of the local, regional,

    and next generation attenuation (NGA) ground-motion prediction equations and determine

    their applicability for northern Iran. Two different statistical approaches, namely the

    likelihood method (LH) of Scherbaum et al. (Bull Seismol Soc Am 94:341348, 2004) and

    the average log-likelihood method (LLH) of Scherbaum et al. (Bull Seismol Soc Am

    99:32343247, 2009), have been applied for evaluation of these models. The best-fitting

    models (considering both the LH and LLH results) over the entire frequency range of

    interest are those of Ghasemi et al. (Seismol 13:499515, 2009a) and Soghrat et al.

    (Geophys J Int 188:645679, 2012) among the local models, Abrahamson and Silva

    (Earthq Spectra 24:6797, 2008) and Chiou and Youngs (Earthq Spectra 24:173215,

    2008) among the NGA models, and finally Akkar and Bommer (Seism Res Lett

    81:195206, 2010) among the regional models.

    Keywords Ground-motion prediction equations Evaluation of fitness Ranking PSHA Northern Iran

    1 Introduction

    The treatment of uncertainty is the greatest challenge in the current probabilistic seismic

    hazard analysis (PSHA) and is an active area of research. It is well known that uncertainty

    H. Zafarani (&)International Institute of Earthquake Engineering and Seismology (IIEES), No. 26, Arghavan St.,North Dibajee, Farmanieh, P.O. Box 19395/3913, Tehran, Irane-mail: [email protected]; [email protected]

    M. MousaviDepartment of Civil Engineering, Faculty of Engineering, Arak University, Arak, Iran

    123

    Nat HazardsDOI 10.1007/s11069-014-1151-2

  • can be divided into two main categories: epistemic (uncertainty in scientific knowledge)

    and aleatory (Toro et al. 1997; Budnitz et al. 1997). Currently, in the classical PSHA

    approach (McGuire 1978), the aleatory uncertainty is dealt with using the basic assumption

    of normal distribution of errors around the mean value of GMPEs and the use of multiple

    relations through a logic tree framework (Budnitz et al. 1997) allows for the assessment of

    epistemic uncertainty. Therefore, the selection of GMPEs and determination of their

    weights in a logic tree analysis is a major part of any seismic hazard analysis (see e.g.,

    Bommer and Scherbaum 2008) and is a matter of debate.

    The branch weights in a logic tree framework correspond to the degree of belief of

    experts in different prediction models. However, due to the lack of domestic experienced

    experts in many regions such as Iran, reliability of expert opinion approach is ques-

    tionable. Because of this concern, in a recent study (Mousavi et al. 2012) by using a set of

    recorded ground-motion data, comparisons are made between a set of candidate ground-

    motion models in the Zagros region of Iran. The candidate models were chosen from three

    categories: local models that were developed based on the local data, regional models

    corresponding to Europe and Middle East datasets, and finally the next generation atten-

    uation (NGA) models (Power et al. 2008). The computed residuals with respect to different

    ground-motion models were analyzed by using the LH and LLH methods of Scherbaum

    et al. (2004, 2009) to rank the different models. One of the most significant results of their

    study was that the regional and local ground-motion models show more consistency with

    the observed data than do the NGA models.

    From the seismotectonic point of view, Iran has been divided into several units (e.g.,

    Takin 1972; Nowroozi 1976; Berberian 1976 and Mirzaei et al. 1998). Different seismo-

    tectonic and geological characteristics between Zagros and northern Iran [mainly consists

    of the Alborz mountain ranges (see Fig. 1)] are the common feature within all these

    studies. Thus, the source spectra, path attenuation and site effects attributed to seismo-

    tectonic styles, may vary between the mentioned regions. On the other hand, some earlier

    studies have claimed that in a broad framework, all parts of Iran can be treated as one unit

    (Chandra et al. 1979) and some authors (e.g., Zafarani et al. 2008; Ghasemi et al. 2009a)

    derived attenuation relations for the Iranian plateau as a whole. However, more recently,

    detailed strong motion studies of Zafarani et al. (2012), Zafarani and Hassani (2013) have

    shown different stress drops for the Zagros and northern Iran regions. The estimated values

    of stress drops for the northern Iranian earthquakes have a higher mean value of 135 bars

    (Zafarani et al. 2012) in comparison with a low value of 66 bars for the Zagros region

    (Zafarani and Hassani 2013). This fact was expected since the majority of the northern

    Iranian database consists of midplate earthquakes that occur more than 500 km from plate

    margins. In contrast, the Zagros region is near the boundary of the Arabian and Eurasian

    plates, and the earthquakes in this region should behave more like interplate events (see

    Zafarani and Soghrat 2012 for more details).

    Cotton et al. (2006) describe how source characteristics, path effects related to geo-

    metric spreading and anelastic attenuation and site effects can vary from region to region.

    Those underlying physics ideally should be manifest in how a GMPE represents the scaling

    of a particular ground-motion intensity measure with respect to magnitude, distance, and

    site condition. Taking into account the above discussion, here we try to perform statistical

    LH and LLH test on a set of GMPEs to assess their suitability and performance for the

    northern Iran region. Following Soghrat et al. (2012), in this study, the whole region of

    northern Iran (including Azerbaijan-Alborz and Kopeh Dagh) is taken into account as one

    single region (see Fig. 1). This assumption increases the total number of records in the

    database, which in return provides more robust results.

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  • 2 Ranking criterion for GMPEs

    2.1 Regional dependency of GMPEs

    The regional variability of ground motions is currently a matter of debate, mainly due to

    the lack of sufficient data. The issue eventually can be solved as newer local models

    become available in all tectonic regions (Stafford et al. 2008; Beauval et al. 2012). Some

    authors assume that ground motions are not regionally dependent, at least for moderate-to-

    large magnitudes (e.g., Stafford et al. 2008). Contrary, other authors have emphasized

    significant regional dependency (e.g., Atkinson and Morrison 2009).

    Currently, there are a large number of published ground-motion models in the literature

    (Douglas 2011). However, the selection and ranking of appropriate models for a particular

    target area usually raises serious practical concerns. The main question is that given a set of

    data recorded in a specified region, how can one quantitatively judge different candidate

    ground-motion models? The approach termed, analysis of variance, was applied by

    Douglas (2004a) to compare ground motions for five local regions within Europe; Douglas

    (2004b) also compared ground motions from Europe, New Zealand, and California. The

    procedure involved calculating and comparing the mean and variance of the log of data

    inside particular magnitude and distance bins for two different regions (e.g., Europe and

    California) and combined data for those regions. Using this approach, Douglas (2004b)

    found more rapid distance attenuation in Europe than California. The visual inspection of

    different GMPEs to see whether there is a significant difference between medians is

    another simple approach that has been used in order to compare the GMPEs in different

    Fig. 1 Major seismotectonic regions of Iran. The northern Iranian earthquakes used in the current study arealso shown (circles)

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  • regions (see e.g., Stafford et al. 2008; Scasserra et al. 2009). Stafford et al. (2008) based

    upon an application of the likelihood approach of Scherbaum et al. (2004) declared that the

    NGA models may confidently be applied for most engineering applications within Europe.

    They also point out to the potential benefits of merging the NGA and European datasets.

    Similar approaches have been used for relatively small numbers of records from parts of

    Europe by Hintersberger et al. (2007) and Drouet et al. (2007); the latter study confirmed

    the application of global GMPEs to regions outside their zone of origin (i.e., host region),

    while the former drew opposite conclusion.

    2.2 The LH and LLH methods for goodness-of-fit analysis

    A practical technique to distinguish between different models and judge their validity is the

    simple statistical analysis of residuals. GMPEs are commonly expressed in terms of log-

    arithmic quantities; hence, the normalized residual is defined as the difference between the

    logarithm of the observations and the logarithm of the model predictions, divided by the

    corresponding standard deviations of the logarithmic model.

    r logSAobs logSAprerSA

    1

    where SAobs, SApre, and rSA represent the observed acceleration response spectra in aspecified period, the median model prediction of the response spectra, and the total stan-

    dard deviation (i.e., combination of inter- and intraevent standard deviations) of the model,

    respectively. Ideally, the so defined residual has a standard normal distribution with zero

    mean and unit variance. The compatibility of the applied ground-motion model with the

    recorded data is defined as the fitness degree of the residuals to this distribution. Statistical

    tests can be utilized to examine the hypothesis that the mean of the residuals is zero and/or

    to test the residuals for unit variance (Montgomery and Runger 2003).

    The likelihood-based measure (LH) has been recently emerged as another comple-

    mentary goodness test which is not only suitable for measuring the model fit, but also for

    testing the underlying statistical assumptions (Scherbaum et al. 2004). For instance, if the

    original distribution follows a perfect standard normal distribution with the zero mean and

    the unit variance, then the corresponding LH transform has a perfectly uniform distribution

    with median value equal to 0.5. Any deviation in the mean, the standard deviation, and the

    shape of the residual distribution corresponds to a specified distribution, the median, and

    the standard deviation of LH values. By using the LH distribution in combination with a

    few simple measures, Scherbaum et al. (2004) have proposed a scheme to assess the

    performance of different ground-motion models. According to this scheme, the ground-

    motion models are categorized into four classes:

    In order to rank a ground-motion model in the lowest accepted capability class (C), themodel has to possess a minimum median LH value of 0.2, and an absolute value for the

    mean and the median of the normalized residuals, and their standard deviations of less

    than 0.75. In addition, the normalized sample standard deviation is required to be less

    than 1.5.

    The model with rank of intermediate capability class (B) is required to possess amedian LH value of at least 0.3, an absolute value of mean and median of the

    normalized residuals and their standard deviations, less than 0.5, and their normalized

    sample standard deviation less than 1.25.

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  • For a model to be ranked in the highest capability class (A), the median LH value mustbe at least 0.4, the absolute value of both measures of the central tendency of the

    normalized residual distribution and their standard deviations must not deviate by more

    than 0.25 from zero. Besides, the normalized sample standard deviation must be less

    than 1.125.

    A model that does not meet the criteria for any of these categories is rankedunacceptable or class D.

    One of the deficiencies of the above-mentioned LH method is that it still requires a few

    subjective decisions, e.g., thresholds for acceptability. The dependency of the results on the

    sample size is another drawback of this method. To avoid these shortcomings, Scherbaum

    et al. (2009) employed a modern information-theoretic approach that is more general than

    the LH method and at least in theory does not depend on ad hoc assumptions such as size of

    samples and significant thresholds. Information theory represents an approximate data-

    driven approach for model selection and ranking in which model performance can be

    expressed by the relative likelihood of a model with respect to the complete candidate set.

    The quantitative decision, favoring different candidate models, requires a meaningful

    measure to distinguish candidate probabilistic models. Within an information theory

    framework, this measure is given by the KullbackLeibler distance (Delavaud et al. 2009).

    The distance quantitatively represents the amount of information loss if the first model

    (i.e., true model) is substituted by the second model (i.e., approximate model). The key

    ingredient, the KullbackLeibler distance, can be estimated from the statistical expectation

    of log-likelihoods of observations for the models under consideration. This latter estimator,

    LLH, is used here as ranking criterion in an information theory framework. In this study,

    the information-theoretic approach in combination with the LH method is used to evaluate

    the compatibility of the candidate ground-motion models with the ground-motion data

    recorded in the northern Iran region. Finally, it should be noted that other statistical tests

    have been proposed/used for selecting and ranking of ground-motion prediction equations.

    For example, the NashSutcliffe model efficiency coefficient (E), a commonly used sta-

    tistic in hydrology (Nash and Sutcliffe 1970), has been used recently by Kaklamanos and

    Baise (2011) to quantitatively compare the predictive capabilities of the NGA models and

    their predecessors. According to Kaklamanos and Baise (2011), the value of E may vary

    between -? and 100 %; when E is less than zero, the arithmetic mean of the observedvalues has greater prediction accuracy than the model itself. The numerical values of E

    may be used to compare alternative models, with higher values indicating better agreement

    between observations and predictions. However, though E adequately quantifies the

    accuracy of the median predicted values, it does not address the standard deviation rela-

    tionships. Also, Kale and Akkar (2013) have introduced an Euclidean distance-based

    ranking procedure based on the concept of the Euclidean distance for ranking of GMPEs

    under a given set of observed data.

    3 The testing dataset and candidate GMPEs

    To test the applicability of candidate ground-motion models, we used horizontal compo-

    nents of 163 three-component records of 32 earthquakes with magnitude ranging from Mw4.9 to 7.4 in northern Iran. In the database, records with hypocentral distances less than 200

    km are chosen and only earthquakes whose moment magnitude estimates are available

    have been used.

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  • In the absence of shear-wave (S-wave) velocities, empirical methods may be employed

    to estimate site classifications (see e.g., Zare et al. 1999; Ghasemi et al. 2009b). However,

    following Soghrat et al. (2012) for reducing uncertainties in this research, only those

    records are considered that their average S-wave velocity to a depth of 30 m (VS30) is

    specifically determined in their stations. However, it should be kept in mind that even with

    an available measure of VS30, there are still remaining uncertainties, e.g., method used for

    estimating VS30, uncertainty on the VS30 estimates and using VS30 that is only a proxy for

    site effects (see e.g., Lee and Trifunac 2010).

    The dataset has been recorded on the Iranian Strong Motion Network of the Building

    and Housing Research Center (http://www.bhrc.ac.ir/ISMN/Index.htm). Table 1 shows the

    information about each of the events with the corresponding reference. The name, code

    number, epicentral distance, and VS30 of these stations are listed in the Appendix Table 7.

    The uncorrected acceleration time series recorded by a given station were corrected for the

    instrument response and baseline, following a standard algorithm (Trifunac and Lee 1973).

    Multi-resolution wavelet analysis (Ansari et al. 2010) was performed to remove undesir-

    able noise from the recorded signals. The characteristics and capabilities of the modified

    nonlinear adaptive wavelet de-noising method for correction of highly noisy strong motion

    records are described in detail by Ansari et al. (2010). According to Ansari et al. (2010),

    displacement response spectra of wavelet de-noised records are more stable than con-

    ventional filtered records with respect to different correction functions and a large number

    of noisy acceleration records that are usually discarded from sets of records used for

    estimating the ground motions can be corrected using this new method.

    Figure 2 shows the magnitude-distance distribution of the employed ground-motion

    records. The different stations are categorized into two different soil classes (Zare et al.

    1999): Rock for VS30 [ 500 m/s and soil for VS30 \ 500 m/s as shown in Fig. 2. The siteclassifications used in the models considered are not identical; nevertheless, the compar-

    isons are made for comparable site classes. For example, Soghrat et al. (2012) and Ghasemi

    et al. (2009a) use a binary site classification, and therefore, we have grouped the sites into

    two classes, i.e., VS30 [ 500 m/s and soil for VS30 \ 500 m/s; while the selected NGAmodels and Kalkan and Gulkan (2004) use site terms that are continues functions of VS30and thus for each station, the corresponding value of V S30 has been used to derive the

    related site response term.

    As it is clear from Fig. 2, the dataset does not include records with Mw [ 6.5 andR \ 90 km, except the one that recorded in the Ab-bar station during the Rudbar M7.4earthquake of June 20,1990 (see Appendix Table 7).

    The candidate ground-motion models are firstly introduced in the following section.

    Then their fitness to the current dataset is analyzed. Cotton et al. (2006) described in detail

    the criteria that should be used primarily as a way of avoiding unintended subjectivity in

    the process of selecting the GMPE models before the data testing. Also, we have taken into

    account some of the updates of these rejection criteria proposed by Bommer et al. (2010).

    We have selected 9 GMPEs derived for different shallow active crustal regions

    worldwide, based on the criteria defined by Cotton et al. (2006) that reject candidate

    models if: (1) the model is derived for an irrelevant tectonic environment, (2) the model is

    not published in a peer-reviewed journal, (3) the dataset used to derive the model is not

    clearly presented, (4) the model has been superseded by a more recent publication, (5) the

    model does not provide predictions over the entire frequency range of interest to engineers,

    (6) the functional form of the model is not appropriate, and (7) the coefficient of the model

    was not determined with a suitable regression method.

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    http://www.bhrc.ac.ir/ISMN/Index.htm

  • Taking into account the update of these rejection criteria by Bommer et al. (2010) and to

    avoid any inconsistencies caused by magnitude conversion formulas (as different GMPEs

    use different magnitude scales), the dataset was restricted only to the events with available

    moment magnitude and the GMPEs which are based on the moment magnitude scale were

    only selected. Also, the models with limited range of applicability (too small to be useful

    for PSHA analysis) have been excluded. We have also taken into account some of the

    Table 1 List of earthquakes used in this study

    Event no. mm/dd/yyyy hh:mm:ss Latitude () Longitude () M w Focal depth Reference

    1 07/22/1980 05:17:06 37.322 50.262 5.6 25 E06

    2 10/29/1985 13:13:40 36.68 54.772 6.1 13 P94

    3 06/20/1990 21:00:11 36.997 49.222 7.4 12 C94

    4 06/24/1990 09:46:01 36.839 49.408 5.3 15 E06

    5 07/06/1990 19:34:54 36.864 49.298 5.3 20 E06

    6 11/28/1991 17:19:53 36.827 49.589 5.6 8 J02

    7 10/15/1995 06:56:34 37.03 49.473 5.2 25 E06

    8 02/04/1997 09:53:53 37.681 57.275 5.5 13 J02

    9 02/04/1997 10:37:47 37.729 57.312 6.5 6 J02

    10 02/05/1997 07:53:45 37.589 57.481 5.2 16 E06

    11 02/28/1997 12:57:45 38.109 48.07 6.1 9 J02

    12 03/02/1997 18:29:42 37.995 47.892 5.3 10 E06

    13 07/09/1998 14:19:18 38.728 48.528 6 ?? J02

    14 08/04/1998 11:41:59 37.223 57.338 5.3 19 E06

    15 11/08/1999 21:37:23 35.699 61.224 5.5 9 E06

    16 11/19/1999 04:40:24 37.321 54.405 5.4 26 E06

    17 11/26/1999 04:27:24 36.953 54.896 5.3 10 E06

    18 08/16/2000 12:53:02 36.706 54.366 4.9 16 E06

    19 06/22/2002 02:58:20 35.597 49.02 6.5 10 W05

    20 05/28/2004 12:38:46 36.258 51.566 6.3 22 T07

    21 03/27/2004 01:31:22 36.74 54.89 5 14 BHRC

    22 05/29/2004 09:23:48 36.489 51.395 5.2 14 E06

    23 05/30/2004 01:42:43 36.27 51.48 4.9 10 BHRC

    24 05/30/2004 19:27:01 36.518 51.595 4.9 7 E06

    25 08/21/2004 03:32:44 37.827 57.647 5.1 15 E06

    26 10/07/2004 21:46:18 37.141 54.466 5.6 28 E06

    27 10/08/2004 13:45:55 37.214 54.499 4.9 32 E06

    28 01/10/2005 18:47:30 37.46 54.53 5.3 29 E06

    29 07/11/2007 06:51:12 38.79 48.60 5.3 25 HRVD

    30 05/27/2008 06:18:08 36.58 48.75 5 14# BHRC

    31 07/03/2008 23:10:06 35.5 58.6 5.1 12 HRVD

    32 09/02/2008 20:00:56 38.68 45.82 5 15 HRVD

    P94 Priestley et al. (1994), C94 Campos et al. (1994), J02 Jackson et al. (2002), W05 Walker et al. (2005),T07 Tatar et al. (2007), E06 Engdahl et al. (2006), HRVD Harvard Seismology (2011), BHRC Building andHousing Research Centre# This value is based on the IIEES report

    Nat Hazards

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  • updates of these rejection criteria by Bommer et al. (2010), aiming to identify robust and

    well-constrained models based on new quality standards in the formulation and derivation

    of models as well as in their applicability range in terms of frequency, magnitude, and

    distance. Cotton et al. (2006) and Bommer et al. (2010) also recommend excluding models

    which lack either nonlinear magnitude dependence or magnitude-dependent decay with

    distance (non-physical models). This issue should be considered just by empirically

    developed models, not by finite source stochastic models (e.g., Soghrat et al. 2012). Their

    results show that the simple models with a constant magnitude scaling cannot be extrap-

    olated to magnitude and distances that are not well represented in the dataset used to derive

    them. According to Cotton et al. (2006), empirical ground-motion models with constant

    magnitude scaling that are calibrated on a large-magnitude dataset will overestimate the

    ground motion from small earthquakes, if extrapolated outside the magnitude range sup-

    ported by the model-generating dataset.

    The abbreviations of the models are given in the second column of Table 2. From the 9

    GMPEs that we have used here, SKZ12, Getal09, and KG04 do not use style-of-faulting as

    a predictor variable and have a binary soil/rock classification; therefore, do not satisfy the

    criteria number 8 of Bommer et al. (2010). The SKZ12 also uses epicentral distance which

    rejects the criteria number 8 of Bommer et al. (2010). The three GMPEs were, however,

    retained because a recent study has shown the good performance of local GMPEs in the

    Zagros region of Iran (Mousavi et al. 2012). Also, according to Bommer et al. (2010), if the

    hazard analysis is to be performed with software that models earthquake occurrences

    within area sources as points without simulated fault ruptures for larger earthquakes (as is

    the common practice in Iran), then in a sense it would be more appropriate to adopt

    GMPEs based on epicentral or hypocentral distance. However, it should be noted that the

    hazard analysts in Iran will certainly soon move to other codes able to take into account the

    extension of faults (e.g., OpenQuake developed within the Global Earthquake Model

    project; http://www.globalquakemodel.org/get-involved/news/openquake/). The Getal09 is

    not including response spectra for T = 0.0 (PGA) and therefore does not provide spectral

    predictions for an adequate range of response periods, chosen here to be from 0.0 to 2.0 s.

    Fig. 2 The magnitudedistance distribution of the employed records used in this study

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    http://www.globalquakemodel.org/get-involved/news/openquake/

  • Therefore, Getal09 satisfy the above stated rejection criteria number 5 of Cotton et al.

    (2006). However, we decide to keep it in the candidate GMPEs, considering its good

    performance in the Zagros region of Iran (Mousavi et al. 2012).

    Candidate ground-motion models were selected from three categories: (1) Ground-

    motion models developed specially for the region of Iran, (2) ground-motion models

    developed for the Middle East-Europe region, and (3) global ground-motion models

    developed by the Next Generation of Ground-Motion Attenuation Models (NGA)

    project (Power et al. 2008). The valid range of frequency, magnitude, and distance for

    these models, accompanying with the distance type, horizontal component definition, and

    host region is indicated in Table 2. All the GMPEs tested using entire database without

    considering their distance limitations. However, this is not a crucial issue, because only

    two GMPEs (i.e., Getal09 and AB10) have a distance validity range of less than 200 km.

    Different horizontal component definitions have been used in the selected GMPEs; most of

    which are simple geometric mean and rotation-independent average horizontal component

    (GMRotI50) defined by Boore et al. (2006) (see Table 2). Here, we do not try to convert

    estimations of different horizontal component definitions to simple geometric mean of

    horizontal components. The geometric mean of horizontal components has been used for

    all GMPEs, except one (i.e., KG04) taking into account that some studies have shown that

    at all periods the ratio of this measure of horizontal components over the new geometric

    mean (GMRotI50) used in the NGA and Ghasemi et al. (2009a) models is near unity (see

    Beyer and Bommer 2006). However, since there is a considerable difference (*10 %)between geometric mean and larger horizontal component (Beyer and Bommer 2006),

    when testing the KG04 predictive model, the larger spectral value of two horizontal

    components is compared with the estimation of the KG04 model.

    The NGA project has developed a series of ground-motion models intended for

    application to geographically diverse regions; the only constraint is that the region be

    tectonically active with earthquakes occurring in the shallow crust (Power et al. 2008).

    Five sets of ground-motion models were developed by teams working independently but

    interacting with one another throughout the development process. Here, the NGA models

    of Boore and Atkinson (2008), Campbell and Bozorgnia (2008), Chiou and Youngs (2008),

    and Abrahamson and Silva (2008) are compared with the Iranian strong motion database.

    We excluded Idriss (2008) due to its lack of a site term. A significant fraction of the

    northern Iranian data has soil site conditions, and hence, the use of a site term is necessary.

    According to Kaklamanos et al. (2011), when employing the NGA models, users routinely

    face situations in which some of the required input parameters are unknown. They have

    presented a framework for estimating the unknown source, path, and site parameters when

    implementing the NGA models in engineering practice. Also, they have derived geomet-

    rically based equations relating the three distance measures found in the NGA models.

    Here, the general strategy was to constrain the input parameters by making the best use

    of available local information where this is available and, if not, using reasonable argu-

    ments and previous experiences elsewhere to adopt the best plausible set of input

    parameters following Kaklamanos et al. (2011). Four different distance measures are used

    in the examined ground-motion relations: Rrup, the shortest distance between the station

    and the rupture surface (AS08, CB08 and CY08), Rjb, the JoynerBoore distance that is the

    closest horizontal distance to the surface projection of the causative fault (AC10, AB10,

    KG04 and BA08), Repi, epicentral distance (SKZ12) and Rhypo, hypocentral distance

    (Getal09). Horizontal distance from the station to the top edge of the rupture measured

    perpendicular to the strike of the fault (Rx) has been also used in the AS08 and CY08

    relations as a supplementary distance measure, as part of the hanging-wall scaling.

    Nat Hazards

    123

  • For moderate events (i.e., Mw \ 6.0), the epicentral, Repi, and hypocentral distances,Rhypo, are used instead of Rjb and Rrup, respectively, since the causative faults cannot be

    well constrained. For the 2004 Baladeh earthquake (Mw 6.2), high-quality, locally recorded

    aftershock data (Tatar et al. 2007) have been used to constrain the fault plane geometry.

    This was also the case for the 2002 Avaj earthquake (Mw 6.3) which well-recorded af-

    tershocks (Tatar et al. 2004) have been used to determine the spatial extent of the fault

    plane. For the Rudbar Mw7.4 earthquake of June 20, 1990, which is the largest event in the

    database, Berberian et al. (1992) have mapped a pattern of discontinuous surface ruptures

    over a length of *85 km. However, the aftershocks distribution does not help in identi-fying the earthquake fault because they were spread over a large area that extends well to

    the north of the fault traces identified by Berberian et al. (1992). As reported by Berberian

    et al. (1992), the spatial correlation between these aftershock locations and the mainshock

    isoseismals was also very poor. Therefore, our fault distances were calculated from the

    Berberian et al. (1992) model with an approximate dip angle of *80 (Campos et al. 1994)along the whole length of the fault. For remaining four earthquakes with Mw C 6.0 (i.e.,

    Table 2 Candidate ground-motion prediction equations

    Model Reference Abbreviations* Main region Component# Frequencyrange (Hz)

    Mw:minmax

    Distance(km)

    Soghrat et al.(2012)

    SKZ12 North of Iran PGAGM,PSAGM

    0.5020.0 4.67.4 REPI3200

    Ghasemi et al.(2009a, b)

    Getal09 Iran PSA inGMRotI50

    0.3320.0 5.07.4 RHYP0100

    Akkar andCagnan (2010)

    AC10 Turkey PGAGM,PGVGM,PSAGM

    0.5033.3 5.07.6 RJB0200

    Akkar andBommer(2010)

    AB10 Europe,Middle East

    PGAGM,PGVGM,PSAGM

    0.3320.0 5.07.6 RJB0100

    Kalkan andGulkan (2004)

    KG04 Turkey PGAMax,PSAMax

    0.5010.0 4.07.4 RJB1.2250

    Abrahamson andSilva (2008)

    AS08 Western USAandCalifornia

    PGA, PGV,PSA inGMRotI50

    0.1100.0 5.08.5 RRUP0200

    Boore andAtkinson(2008)

    BA08 Western USAandCalifornia

    PGA, PGV,PSA inGMRotI50

    0.1100.0 5.08.0 RJB0200

    Campbell andBozorgnia(2008)

    CB08 Western USAandCalifornia

    PGA, PGV,PSA inGMRotI50

    0.1100.0 4.08.5 RRUP0200

    Chiou andYoungs (2008)

    CY08 Western USAandCalifornia

    PGA, PGV,PSA inGMRotI50

    0.1100.0 4.08.5 RRUP0200

    * Abbreviations of GMPEs used in the current study# GMRotI50, rotation-independent average horizontal component (Boore et al. 2006); subscripts Max andGM, maximum and geometric mean of horizontal components, respectively REPI Epicentral distance, RRUP Rupture distance, RJB JoynerBoore distance, RHYP Hypocentral distance

    Nat Hazards

    123

  • event numbers 2, 9, 11, and 13 in Table 1), there was no information on the spatial extent

    of the rupture,; therefore, the empirical relations of Wells and Coppersmith (1994) for all

    fault types have been used to define the rupture planes assuming that the hypocenters are

    located at the middle.

    Regarding Rx, which is used in the AS08 and CY08 models for quantifying the

    hanging-wall, we also follow the Kaklamanos et al. (2011) formulation that is based on an

    important location measure, the source-to-site azimuth, and Rjb (see Fig. 2 in Kaklamanos

    et al. 2011). It is worth to say that the hanging-wall effects and details of fault rupture plane

    is not crucial in the current study, taking into account the magnitude-distance distribution

    of database that is dominated by far-field records from moderate events (see Fig. 2).

    Also, the regional values of depth to Vs = 1.0 km/s (Z1.0 for AS08 and CY08) and

    depth to Vs = 2.5 km/s (Z2.5 for CB08) have been adopted from crustal velocity studies

    in the region (Ashtari et al. 2005; Abbassi et al. 2010; Radjaee et al. 2010; Moradi et al.

    2011) in combination with the Chandler et al. (2005) method. Based on a large amount

    of velocity data, along with thickness of sedimentary and crystalline layers within

    bedrockcollected from all over the worldChandler et al. (2005) has proposed a

    methodology, which can be used at the regional level to develop an averaged S-wave

    velocity profile for a geological region. In this study, the above approach has been used

    to estimate the velocity gradient in the crust (see Fakhimnia et al. 2013 for details).

    Alternatively, one can use the empirical relations between Z1.0 and Z2.5 with VS30 that

    has been proposed by Chiou and Youngs (2008) and Campbell and Bozorgnia (2008),

    respectively. This approach has been adopted by Scasserra et al. (2009) during com-

    parison of the NGA GMPEs to Italian database. However, using such empirical relations

    developed based on the NGA database (mainly from California), implicitly assumes the

    similar velocity gradient in rock for California and studied area sites, which may not be

    correct.

    The minimum depth of seismogenic rupture (ZTOR) is a controversial topic, and little

    guidance exists in the literature on its estimation. The method suggested by Kaklamanos

    et al. (2011) is used to estimate ZTOR from the hypocentral depth (ZHYP), down-dip rupture

    width (W), and dip angle (d), assuming that the hypocenter is located 60 % down the fault

    width:

    ZTOR maxZHYP 0:6 W sin d; 0 2Also, a minimum depth of 1 km was imposed considering the lack of surface rupture for

    the analyzed eventsRudbar earthquake is an exceptionand assuming that depths above

    1 km did not radiate significant seismic radiation in the frequency range we are considering

    here (see e.g., Campbell 1997).

    The detailed comparisons made by Akkar and Cagnan (2010) between a combined

    Italian and Turkish accelerometric dataset and different GMPEs have shown that depth can

    be of importance for delineating the differences between local and global GMPEs.

    Therefore, in the current study, the published focal depths determined by body-waveform

    modeling as the most accurate ones have been used if they were available (see Table 1).

    For 17 moderate events, the results of Engdahl et al. (2006) which is based on an advanced

    technique for 1D earthquake relocation have been used. These depths are more precise than

    those available in local and/or international agencies, but less accurate than the body-

    waveform inversions. For remaining six moderate events, the depths reported by inter-

    national or local agencies have been used.

    Nat Hazards

    123

  • 4 Ranking results

    As a preliminary step toward developing goodness-of-fit analysis, for each of the ground-

    motion records described in the Appendix, Table 7 accompanying acceleration response

    Fig. 3 Normalized residual histograms for Sa(T = 1.0 s) with respect to different ground-motion models.Solid line shows the expected distribution function for a standard normal distribution

    Fig. 4 Distribution of LH values for Sa(T = 1.0 s) with respect to different ground-motion models

    Nat Hazards

    123

  • Ta

    ble

    3R

    ank

    ing

    of

    mod

    els

    bas

    edo

    nth

    eL

    Hm

    eth

    od

    for

    dif

    fere

    nt

    per

    iods

    Model

    nam

    eR

    ank

    ME

    DL

    Hr

    ME

    DN

    Rr

    ME

    AN

    NR

    rS

    TD

    NR

    r

    LH

    ranki

    ng,

    PG

    A

    CY

    08

    A0.4

    50.0

    5-

    0.0

    60.1

    5-

    0.0

    40.0

    91.1

    20.0

    7

    AS

    08

    B0.4

    60.0

    3-

    0.4

    90.1

    1-

    0.4

    40.1

    01.0

    50.0

    7

    KG

    04

    B0.4

    60.0

    4-

    0.0

    90.1

    20.0

    40.1

    01.1

    30.0

    7

    AB

    10

    C0.3

    20.0

    50.7

    40.1

    60.7

    50.1

    01.1

    10.0

    7

    BA

    08

    C0.4

    30.0

    60.1

    20.1

    20.1

    80.1

    11.2

    60.0

    8

    SK

    Z12

    C0.4

    80.0

    50.5

    10.0

    90.5

    80.0

    90.9

    50.0

    6

    AC

    10

    D0.2

    20.0

    31.2

    30.1

    11.2

    50.0

    80.8

    90.0

    5

    CB

    08

    D0.2

    70.0

    4-

    0.8

    90.1

    1-

    0.7

    70.1

    11.3

    20.0

    9

    LH

    ranki

    ng,

    T=

    0.1

    s

    AS

    08

    A0.4

    50.0

    6-

    0.1

    00.1

    0-

    0.0

    90.0

    91.0

    70.0

    7

    CY

    08

    B0.4

    20.0

    50.3

    20.0

    80.2

    60.1

    01.1

    50.0

    7

    Get

    al09

    B0.4

    10.0

    40.4

    90.1

    70.3

    70.0

    91.0

    10.0

    6

    KG

    04

    B0.4

    10.0

    4-

    0.0

    80.1

    7-

    0.0

    70.1

    11.2

    10.0

    7

    BA

    08

    C0.3

    50.0

    50.1

    60.1

    10.3

    40.1

    21.2

    90.0

    8

    CB

    08

    C0.3

    40.0

    4-

    0.3

    50.1

    7-

    0.4

    10.1

    21.2

    80.0

    8

    SK

    Z12

    C0.4

    20.0

    40.6

    30.1

    20.6

    60.0

    91.0

    40.0

    6

    AB

    10

    D0.2

    40.0

    51.0

    40.1

    80.9

    20.1

    01.1

    30.0

    7

    AC

    10

    D0.1

    80.0

    21.3

    50.0

    81.3

    50.0

    80.9

    30.0

    6

    LH

    ranki

    ng,

    T=

    0.2

    s

    KG

    04

    A0.5

    20.0

    70.0

    30.0

    90.1

    30.0

    91.0

    80.0

    8

    AS

    08

    B0.5

    10.0

    7-

    0.2

    80.0

    9-

    0.3

    00.0

    91.0

    10.0

    7

    BA

    08

    B0.4

    40.0

    50.2

    10.1

    20.2

    50.1

    11.1

    90.0

    8

    CY

    08

    B0.5

    10.0

    50.3

    00.1

    10.2

    70.1

    01.0

    90.0

    8

    Get

    al09

    B0.5

    20.0

    60.4

    80.0

    90.4

    90.0

    90.9

    80.0

    7

    AB

    10

    C0.4

    30.0

    60.6

    10.1

    00.6

    50.1

    01.0

    70.0

    7

    CB

    08

    C0.3

    30.0

    6-

    0.5

    80.1

    2-

    0.5

    40.1

    11.2

    50.0

    9

    SK

    Z12

    C0.4

    30.0

    60.5

    00.1

    50.5

    10.1

    01.0

    80.0

    7

    Nat Hazards

    123

  • Ta

    ble

    3co

    nti

    nued

    Model

    nam

    eR

    ank

    ME

    DL

    Hr

    ME

    DN

    Rr

    ME

    AN

    NR

    rS

    TD

    NR

    r

    AC

    10

    D0.2

    30.0

    41.1

    50.1

    01.1

    30.0

    80.8

    50.0

    6

    LH

    ranki

    ng,

    T=

    0.5

    s

    CY

    08

    A0.4

    90.0

    30.0

    10.1

    3-

    0.0

    20.1

    01.0

    80.0

    8

    AB

    10

    B0.5

    00.0

    40.3

    00.1

    10.2

    20.0

    80.9

    90.0

    7

    AS

    08

    B0.4

    20.0

    6-

    0.2

    20.1

    4-

    0.3

    30.0

    91.0

    50.0

    7

    BA

    08

    B0.4

    50.0

    6-

    0.1

    50.1

    5-

    0.1

    40.1

    11.1

    90.0

    8

    Get

    al09

    B0.5

    20.0

    40.3

    80.1

    10.3

    90.0

    80.9

    40.0

    7

    SK

    Z12

    B0.5

    30.0

    40.2

    90.0

    90.2

    10.0

    80.8

    70.0

    6

    KG

    04

    B0.5

    30.0

    5-

    0.4

    30.1

    1-

    0.2

    80.0

    80.9

    40.0

    7

    AC

    10

    D0.3

    90.0

    60.8

    10.1

    40.8

    00.0

    80.8

    70.0

    6

    CB

    08

    D0.2

    30.0

    4-

    1.0

    60.1

    7-

    1.0

    30.1

    11.2

    20.1

    0

    LH

    ranki

    ng,

    T=

    0.7

    5s

    AB

    10

    A0.5

    70.0

    50.1

    30.0

    90.0

    90.0

    80.8

    30.0

    6

    AS

    08

    A0.4

    80.0

    30.0

    40.1

    1-

    0.0

    10.0

    91.0

    00.0

    7

    BA

    08

    A0.4

    40.0

    6-

    0.2

    00.1

    0-

    0.2

    10.1

    01.0

    90.0

    7

    CY

    08

    B0.5

    30.0

    4-

    0.0

    40.1

    0-

    0.1

    20.0

    91.0

    10.0

    8

    Get

    al09

    B0.5

    40.0

    30.3

    30.1

    00.3

    10.0

    70.8

    10.0

    6

    SK

    Z12

    B0.5

    50.0

    50.3

    80.0

    70.3

    30.0

    70.7

    80.0

    5

    KG

    04

    B0.5

    20.0

    3-

    0.6

    40.0

    8-

    0.6

    50.0

    70.8

    00.0

    5

    AC

    10

    C0.5

    00.0

    50.6

    00.1

    10.6

    50.0

    70.8

    00.0

    5

    CB

    08

    D0.2

    70.0

    4-

    1.1

    00.1

    1-

    1.1

    60.1

    01.1

    00.0

    8

    LH

    ranki

    ng,

    T=

    1.0

    s

    AB

    10

    A0.5

    60.0

    40.1

    00.1

    10.0

    20.0

    80.8

    30.0

    5

    AS

    08

    A0.5

    10.0

    50.1

    50.1

    10.1

    00.0

    90.9

    90.0

    7

    CY

    08

    A0.5

    10.0

    4-

    0.1

    90.1

    1-

    0.2

    50.0

    91.0

    20.0

    6

    BA

    08

    B0.4

    90.0

    5-

    0.2

    90.1

    2-

    0.3

    20.1

    01.1

    10.0

    7

    Get

    al09

    B0.5

    80.0

    40.2

    20.1

    10.2

    60.0

    70.8

    10.0

    5

    SK

    Z12

    B0.5

    40.0

    50.3

    30.1

    00.3

    20.0

    70.7

    90.0

    5

    Nat Hazards

    123

  • Ta

    ble

    3co

    nti

    nued

    Model

    nam

    eR

    ank

    ME

    DL

    Hr

    ME

    DN

    Rr

    ME

    AN

    NR

    rS

    TD

    NR

    r

    KG

    04

    C0.5

    40.0

    3-

    0.5

    10.0

    7-

    0.5

    70.0

    70.7

    70.0

    5

    AC

    10

    C0.5

    30.0

    50.5

    10.0

    80.5

    10.0

    70.8

    10.0

    5

    CB

    08

    D0.2

    40.0

    4-

    1.1

    80.1

    1-

    1.2

    30.1

    01.1

    00.0

    7

    LH

    ranki

    ng,

    T=

    1.5

    s

    AB

    10

    A0.5

    10.0

    3-

    0.0

    70.1

    2-

    0.1

    00.0

    80.9

    20.0

    6

    AS

    08

    A0.4

    90.0

    60.1

    80.1

    20.1

    80.0

    91.0

    50.0

    7

    Get

    al09

    A0.6

    00.0

    5-

    0.0

    50.1

    0-

    0.1

    00.0

    80.8

    40.0

    6

    SK

    Z12

    A0.5

    30.0

    40.1

    20.1

    20.1

    10.0

    80.8

    90.0

    6

    AC

    10

    B0.5

    30.0

    40.3

    80.0

    90.4

    30.0

    80.8

    70.0

    5

    CY

    08

    B0.4

    50.0

    6-

    0.2

    20.1

    3-

    0.3

    00.1

    01.1

    30.0

    7

    KG

    04

    C0.4

    80.0

    5-

    0.6

    20.1

    0-

    0.6

    40.0

    80.9

    10.0

    6

    BA

    08

    C0.4

    10.0

    5-

    0.4

    50.1

    4-

    0.4

    90.1

    01.1

    40.0

    8

    CB

    08

    D0.2

    50.0

    5-

    1.0

    90.1

    4-

    1.2

    50.1

    01.2

    10.0

    8

    LH

    ranki

    ng,

    T=

    2.0

    s

    AB

    10

    A0.5

    40.0

    4-

    0.1

    00.1

    2-

    0.1

    40.0

    80.9

    10.0

    6

    Get

    al09

    A0.5

    40.0

    30.1

    80.1

    10.1

    30.0

    70.8

    10.0

    6

    SK

    Z12

    A0.5

    20.0

    5-

    0.0

    70.1

    4-

    0.1

    00.0

    80.9

    10.0

    6

    AC

    10

    B0.5

    00.0

    50.4

    10.0

    80.4

    40.0

    80.8

    80.0

    5

    AS

    08

    B0.4

    20.0

    60.3

    30.1

    00.3

    10.1

    11.1

    20.0

    8

    CY

    08

    B0.4

    20.0

    6-

    0.1

    70.1

    3-

    0.2

    30.1

    01.1

    60.0

    7

    KG

    04

    C0.4

    40.0

    5-

    0.6

    50.0

    9-

    0.6

    90.0

    90.9

    60.0

    6

    BA

    08

    C0.4

    50.0

    5-

    0.4

    40.1

    4-

    0.5

    20.1

    01.1

    40.0

    7

    CB

    08

    D0.2

    80.0

    7-

    1.0

    60.1

    7-

    1.1

    80.1

    11.2

    40.0

    8

    Nat Hazards

    123

  • spectra, Sa(T), have been calculated at a series of periods (0.0 s (i.e., PGA), 0.1, 0.2, 0.5,

    0.75, 1.0, 1.5, and 2 s) using the selected ground-motion models. The clearest and simplest

    way to identify the presence of potential biases in the model predictions is the visual

    inspection of residual histograms. Using the residuals plots, one is able to identify the

    group of GMPEs which are best-fitting the data and to identify the GMPEs which are

    providing the worse fit to the data. The residual set associated with each model has been

    determined using Eq. (1) for desired periods. For example, the histograms of the residuals

    of the models for period of 1.0 s are shown in Fig. 3. The procedure may be repeated for

    the predetermined periods. The standard normal distribution functions which are expected

    for each set are also plotted for each case in Fig. 3. From inspection of this figure, it is

    apparent that SKZ12, Getal09, AS08, and AB10 have done a better job of predicting

    desired values.

    As a second step, the LH method has been applied to rank ground-motion models into

    four classes A, B, C, and D. Figure 4 shows the distribution of LH values for

    Sa(T = 1.0 s). It is difficult to judge qualitatively which one is more similar to a uniform

    distribution. The quantitative goodness of fit of models to data in this method is evaluated

    by using the median LH values (MEDLH) and the median, mean, and the standard

    deviation of the normalized residuals (MEDNR, MEANNR, and STDNR, respectively).

    The corresponding standard deviations of these measures (r) are calculated using thecomputer-aided statistical technique of bootstrap resampling (Efron and Tibshirani 1993).

    By using these measures and based on the scheme presented in the former sections, the

    ground-motion models are ranked in the categories A, B, C, or D (Table 3). The relative

    similarity of ranking results for different periods may be interpreted as a sign of method

    stability, though some studies have shown that the adequacy between a model and

    observations is depending on the period considered (see e.g., Beauval et al. 2012; Delavaud

    et al. 2012). This hypothesis is examined in Table 3, which shows the LH-based rankings

    of models in different periods. Inspection of the results shows that three models: AS08,

    CY08, and Getal09 are ranked A or B for all considered periods. Another finding is that

    two models CB08 and AC10 are assigned rank D, or unacceptable, six and four times,

    respectively.

    Table 4 Final ranking of models based on the LH method for united residuals

    All periods

    Model name Rank MEDLH r MEDNR r MEANNR r STDNR r

    AS08 A 0.47 0.02 -0.04 0.04 -0.07 0.03 1.07 0.03

    CY08 A 0.47 0.02 -0.01 0.05 -0.05 0.03 1.11 0.03

    Getal09 A 0.52 0.01 0.25 0.04 0.23 0.03 0.92 0.02

    SKZ12 B 0.51 0.02 0.35 0.03 0.33 0.03 0.95 0.02

    KG04 B 0.49 0.02 -0.32 0.04 -0.28 0.03 1.04 0.03

    AB10 B 0.49 0.01 0.32 0.04 0.30 0.03 1.05 0.02

    BA08 B 0.43 0.02 -0.13 0.05 -0.11 0.04 1.22 0.03

    AC10 D 0.36 0.02 0.81 0.05 0.82 0.03 0.93 0.02

    CB08 D 0.27 0.01 -0.92 0.06 -0.95 0.04 1.25 0.03

    Nat Hazards

    123

  • Table 5 Ranking of models based on the information-theoretic (LLH) method for different periods

    Rank LLH Model Rank LLH Model

    PGA (T = 0.0 s) T = 0.1 s

    1 1.54 KG04 1 1.68 AS08

    2 1.55 CY08 2 1.76 Getal09

    3 1.59 BA08 3 1.77 KG04

    4 1.65 AS08 4 1.78 CY08

    5 1.67 SKZ12 5 1.85 CB08

    6 1.68 AB10 6 1.88 BA08

    7 1.97 CB08 7 1.98 SKZ12

    8 2.74 AC10 8 2.31 AB10

    Getal09 9 3.06 AC10

    T = 0.2 s T = 0.5 s

    1 1.63 KG04 1 1.58 CY08

    2 1.64 BA08 2 1.62 KG04

    3 1.65 AS08 3 1.64 BA08

    4 1.66 CY08 4 1.65 SKZ12

    5 1.73 Getal09 5 1.66 AB10

    6 1.74 SKZ12 6 1.68 Getal09

    7 1.85 CB08 7 1.68 AS08

    8 1.95 AB10 8 2.12 AC10

    9 2.61 AC10 9 2.38 CB08

    T = 0.75 s T = 1.0 s

    1 1.46 AB10 1 1.41 AB10

    2 1.50 AS08 2 1.47 AS08

    3 1.52 Getal09 3 1.50 Getal09

    4 1.53 CY08 4 1.56 SKZ12

    5 1.55 SKZ12 5 1.56 CY08

    6 1.58 BA08 6 1.67 BA08

    7 1.68 KG04 7 1.80 KG04

    8 1.92 AC10 8 1.85 AC10

    9 2.44 CB08 9 2.60 CB08

    T = 1.5 s T = 2.0 s

    1 1.49 AB10 1 1.53 AB10

    2 1.52 Getal09 2 1.53 SKZ12

    3 1.53 SKZ12 3 1.55 Getal09

    4 1.59 AS08 4 1.75 AS08

    6 1.76 CY08 6 1.80 CY08

    7 1.89 AC10 7 1.88 AC10

    8 1.89 BA08 8 1.95 BA08

    9 1.96 KG04 9 2.13 KG04

    10 2.84 CB08 10 2.79 CB08

    Nat Hazards

    123

  • In the current PSHA calculations, it is not possible for now to take into account different

    GMPEs depending on their period-dependent efficiency, so there are arguments for

    merging the dataset. Also, since the ranking results are more or less stable for the different

    periods, it has been decided to merge all residuals into a unit set and then repeat the

    ranking procedure. Table 4 shows the ranking of models based on this united residuals set.

    Each period corresponds to a residual vector that the LH and LLH analysis can be per-

    formed on it. Putting all residual vectors together leads to greater residual vector which

    represents the overall behavior of a considered attenuation model. Tables 4 and 6 show the

    results of application of LH and LLH analysis on this residual vector, respectively. Table 4

    can be considered as the final ranking of models based on the LH method. According to

    this ranking, two models CB08 and AC10 should be excluded from the acceptable models.

    Also, two models developed specially for Iran region, Getal09 and SKZ12, are ranked A

    and B, respectively. On the other hand, regarding the regional models that are models

    developed for the Europe and Middle East, only one model, i.e., AB10 show an acceptable

    performance (rank B).

    As the final step of performance analysis, the average sample log-likelihood (LLH) has

    been calculated for each of the seven considered periods, using the Eq. (1). Table 5

    compares the mean LLH values for the candidate ground-motion models in different

    periods. As it is clear, some of the GMPEs are more compatible with the testing database

    for nearly all periods. A final period-independent ranking can be defined based on the

    average LLH values of all periods, as is shown in Table 6. As it is clear, the ranking for the

    top four models is based on very close LLH values (Table 6, 1.61 for Getal09, 1.63 for

    AS08, 1.64 for CY08 and 1.65 for SKZ12) and more robust discrimination among them

    may require more data.

    By comparing the Table 4 with Table 6, the agreement of the LH and the information

    theory method (LLH) in ranking of the models is confirmed. The two models that were

    ranked as D with the LH method are also placed at the bottom of Table 6.

    5 Discussions and conclusions

    The difference between local, regional, and global ground-motion prediction models has

    been investigated in order to determine their applicability for northern Iran. Two different

    Table 6 Final ranking of modelsbased on the information-theo-retic (LLH) method for allperiods

    All periods

    Rank LLH Model

    1 1.61 Getal09

    2 1.63 AS08

    3 1.64 CY08

    4 1.65 SKZ12

    5 1.72 AB10

    6 1.74 BA08

    8 1.77 KG04

    9 2.26 AC10

    10 2.35 CB08

    Nat Hazards

    123

  • approaches have been used here to evaluate candidate ground-motion models. First, by

    using a set of recorded ground-motion data, the computed residuals with respect to

    different ground-motion models were analyzed by using the LH method. Based on this

    method, two models (AC10 and CB08) were unacceptable and the remaining models

    were ranked as A or B. However, it should be noted that there are reliable differences in

    ranking results from one period to the other (i.e., period-dependent ranking), taking into

    account that the number of records for each period is significant. In other words, the

    residuals can be merged, but it gives another result which should not erase the period-

    dependent ranking.

    Second, information theory (LLH) was employed to rank the models, again. The good

    agreement of these two methods confirms the reliability of the final ranking. One of the

    main results of the current study is that some non-indigenous GMPEs show a high degree

    of consistency with the data from northern Iran region (i.e., Abrahamson and Silva 2008;

    Chiou and Youngs 2008). A similar conclusion was made by Delavaud et al. (2012) who

    tested the global applicability of GMPEs for active shallow crustal regions. According to

    Delavaud et al. (2012), some models in particular demonstrated a strong power of geo-

    graphically wide applicability in different geographic regions with respect to the testing

    dataset. Due to a paucity of data, the testing of the method developed here does not include

    data from earthquakes with Mw [ 6.5 and R \ 90 km, except one. Taking into account thelimited number of observations, the issue is open till more strong motion records (par-

    ticularly near-field ones) became available. The conclusions/results are restricted/limited

    (are not rigorous) and should be used with caution. In such situations, the use of physics-

    based models such as Soghrat et al. (2012) should be preferred taking into account their

    more consistency with the physics of earthquakes; though even in such models, there also

    may be significant uncertainties associated with the input parameters required for the

    simulations. Based on the results of the current study, five GMPEs have been proposed for

    PSHA analysis in the region. The best-fitting models (considering both the LH and LLH

    results) over the entire frequency range of interest are those of Ghasemi et al. (2009a) and

    Soghrat et al. (2012) among the local models, Abrahamson and Silva (2008) and Chiou and

    Youngs (2008) among the NGA models, and finally Akkar and Bommer (2010) among the

    regional models.

    Although Turkey and Iran have similar tectonic regimes (shallow active crustal), the

    predictive models derived for Turkey generally are not applicable for Iran (Northern Iran)

    according to the findings of this study. After careful inspection, it is clear that the

    Turkish data of KG04 and AC10 are primarily from western Turkey. Using the coda

    normalization method for the direct S-waves, Horasan and Boztepe-Guney (2004) has

    reported S-wave attenuation in the Sea of Marmara, western Turkey as Qs(f) = 40f1.03,

    while Zafarani et al. (2012) have obtained an average value of Qs(f) = 101f0.8 for

    northern Iran region based on the generalized inversion of the S-wave amplitude spectra.

    This implies that the northern Iranian strong motion data attenuate slower than those of

    western Turkey at low frequencies (i.e., T [ 1 s). This is confirmed by the period-dependent ranking results from the LLH method. As it is clear, the Turkish-based

    attenuation model KG04 has a suitable performance at the T = 0, 0.1, 0.2, 0.5, and

    0.75 s (see Table 3 and 5). However, the model fails to predict northern Iranian data at

    T = 1.0, 1.5, and 2.0 s.

    Regarding the NGA models, recordings from California cover almost 60 % of the BA08

    and CB08 models, while it consist only 40 % of the AS08 and CY08 models (Power et al.

    2008). Also, it is important to recognize the large number of Taiwanese records in the

    AS08 and CY08 models, taking into account the similarity of shear-wave quality factor in

    Nat Hazards

    123

  • the Taiwan (Qs(f) = 125f0.8; Sokolov et al. 2000) and northern Iran regions

    (Qs(f) = 101f0.8; Zafarani et al. 2012). This may be the reason of the better performance of

    the two latter models, i.e., AS08 and CY08 models.

    The similar performance of Ghasemi et al. (2009a), developed based on the whole

    Iranian plateau database, and Soghrat et al. (2012), established specifically for northern

    Iran, may be questionable and surprising. However, it should be taken into account that

    the Scherbaum et al. (2004, 2009) approaches used here assess overall goodness of fit of

    data to a model, i.e., all aspects of the model performance and accuracy are evaluated in

    a lumped manner. If one of the model components was in error, that effect could be

    obscured through compensating errors in the comparison process of normalized residuals

    to the standard normal variate (Scasserra et al. 2009). Accordingly, while the results of

    the current study are promising with respect to the similar performance of Ghasemi

    et al. (2009a) and Soghrat et al. (2012) relations in northern Iran, a formal analysis of

    the adequacy of the models with respect to magnitude scaling, distance scaling, and site

    effects is also needed. The details of this procedure will be published in a separate paper

    (Mousavi et al. 2013). Also, careful inspection shows that the Ghasemi et al. (2009a)

    and the Soghrat et al. (2012) equations are very close in the range of 10100 km (see

    Fig. 15 in Soghrat et al. 2012), which is the dominant distance range of the current

    dataset.

    Regarding our conclusions, it should be taken into account that according to Musson

    (2009), if an empirical GMPE is to be used in probabilistic seismic hazard assessment,

    the model would probably be subject to extrapolate beyond the parameter space within

    which it was constructed, especially for hazard at low annual probabilities, even with the

    proviso that the dataset is reasonably extensive and well selected. In this case, the

    features of the model, especially its functional form, may turn out to have unexpected and

    undesirable implications. Although a ground-motion model may be a correct represen-

    tation of its dataset, the effects of the functional form applied can be such that it becomes

    doubtful whether the model should be used for probabilistic hazard purposes. Therefore,

    although the local model of Ghasemi et al. (2009a) did a good job of prediction for the

    limited database of northern Iran, but care must be taken when using it in a real seismic

    hazard project, especially for low hazard levels; taking into account its simple functional

    form.

    Finally, if we would like to find corresponding weights of different GMPEs to be used in

    PSHA, we may do so by using the procedure suggested by Mousavi et al. (2012). The

    method combines the results of the LH and information theory methods, in two steps.

    These weights provide a quantitative alternative to expert opinions in seismic hazard

    projects and can be used to complement expert opinions, where these may be available or

    replace expert opinions when these are unavailable.

    Acknowledgments The authors acknowledge the Building and Housing Research Centre of Iran forproviding them with the accelerograms and shear-wave velocities used in the current study. This study wassupported by the International Institute of Earthquake Engineering and Seismology (IIEES) funds, ProjectG-05-92: Seismicity and Seismic Hazard Studies for an International Hotel in Tehran, Iran This financialsupport is gratefully acknowledged. Finally, we are very grateful to two anonymous reviewers for theirinsightful and constructive comments, which significantly improved the manuscript.

    Appendix

    See Table 7.

    Nat Hazards

    123

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    66

    R8

    15

    64

    Nah

    avan

    d2

    76

    13

    5.9

    24

    9.5

    28

    64

    R7

    69

    65

    Ab

    har

    27

    63

    36

    .15

    49

    .22

    75

    65

    S2

    91

    66

    Deh

    Jala

    l2

    76

    83

    6.3

    14

    8.7

    20

    87

    R7

    48

    67

    Dar

    seji

    n2

    76

    9/0

    23

    6.0

    24

    9.2

    37

    65

    3R

    63

    6

    68

    Sae

    inG

    hal

    e2

    77

    23

    6.3

    04

    9.0

    73

    97

    8R

    64

    2

    69

    Go

    lT

    app

    eh2

    77

    73

    5.2

    24

    8.2

    32

    10

    0R

    1,0

    77

    70

    Qah

    rvar

    d2

    77

    83

    5.4

    74

    8.0

    68

    81

    08

    S4

    14

    71

    Sh

    irin

    su2

    78

    13

    5.5

    04

    8.4

    61

    77

    63

    R8

    13

    72

    Bak

    Kan

    di

    27

    87

    /03

    36

    .40

    49

    .57

    42

    10

    8S

    30

    8

    Nat Hazards

    123

  • Ta

    ble

    7co

    nti

    nued

    Nu

    mb

    er.

    Sta

    tio

    nn

    ame

    Cod

    eC

    oo

    rdin

    ate

    C.P

    GA

    a(c

    m/s

    /s)

    Hy

    po

    centr

    ald

    ista

    nce

    Sit

    ebV

    S30

    ne

    73

    Ko

    mij

    an2

    82

    13

    4.7

    24

    9.3

    31

    91

    03

    R6

    91

    74

    Far

    mah

    in2

    82

    63

    4.5

    04

    9.6

    82

    01

    42

    R5

    89

    75

    Asa

    d-A

    bad

    28

    80

    34

    .78

    48

    .12

    14

    13

    5R

    74

    3

    76

    Qah

    avan

    d2

    88

    23

    4.8

    54

    92

    38

    3R

    1,0

    98

    77

    Jira

    ndeh

    29

    72

    /01

    36

    .70

    49

    .78

    17

    14

    9S

    46

    2

    78

    Teh

    ran

    18

    32

    95

    35

    .74

    51

    .37

    17

    62

    R5

    11

    79

    Teh

    ran

    56

    33

    02

    35

    .72

    51

    .27

    28

    68

    R6

    13

    80

    Teh

    ran

    24

    33

    04

    35

    .75

    51

    .16

    25

    72

    R5

    22

    81

    Teh

    ran

    52

    33

    11

    35

    .74

    51

    .58

    20

    58

    R5

    93

    82

    Tal

    eqan

    33

    18

    36

    .18

    50

    .76

    12

    09

    0S

    46

    2

    83

    Mar

    dA

    bad

    33

    21

    35

    .73

    50

    .85

    52

    99

    S3

    04

    84

    Bo

    om

    ehen

    33

    23

    35

    .73

    51

    .86

    21

    67

    R6

    96

    85

    Qaz

    vin

    23

    33

    23

    6.2

    45

    0.0

    54

    41

    69

    S*

    86

    Has

    anK

    eyf

    33

    33

    36

    .55

    1.1

    58

    79

    54

    S3

    39

    87

    Kah

    riza

    k3

    33

    43

    5.5

    51

    .37

    26

    87

    S3

    23

    88

    Has

    san

    Ab

    ad3

    34

    33

    5.3

    75

    1.2

    52

    81

    05

    S4

    50

    89

    TE

    HR

    AN

    27

    33

    47

    35

    .74

    51

    .66

    21

    59

    R5

    69

    90

    Bab

    ols

    ar3354

    36.7

    052.6

    62

    5131

    S187

    91

    Nek

    a3

    35

    83

    6.6

    35

    3.2

    81

    61

    95

    S3

    92

    92

    To

    nek

    abo

    n3

    36

    13

    6.8

    15

    0.8

    84

    79

    8S

    25

    2

    93

    Mo

    alem

    Kel

    ayeh

    33

    67

    36

    .45

    50

    .47

    29

    11

    24

    S4

    90

    94

    No

    shah

    r3

    36

    8/0

    13

    6.6

    55

    1.4

    91

    05

    44

    S1

    65

    95

    No

    or

    33

    69

    /01

    36

    .57

    52

    .01

    58

    60

    S1

    78

    96

    Ro

    od

    sar

    33

    73

    37

    .14

    50

    .28

    52

    17

    3S

    24

    0

    Nat Hazards

    123

  • Ta

    ble

    7co

    nti

    nued

    Nu

    mb

    er.

    Sta

    tio

    nn

    ame

    Cod

    eC

    oo

    rdin

    ate

    C.P

    GA

    a(c

    m/s

    /s)

    Hy

    po

    centr

    ald

    ista

    nce

    Sit

    ebV

    S30

    ne

    97

    No

    zar

    Ab

    ad3

    37

    43

    6.8

    05

    3.2

    52

    41

    97

    S4

    38

    98

    Ban

    dar

    -e-K

    yas

    hah

    r3398

    37.4

    249.9

    33

    0200

    S184

    99

    Sae

    idA

    bad

    34

    04

    35

    .67

    51

    .19

    26

    78

    R9

    21

    10

    0E

    stal

    kh

    Po

    sht

    34

    11

    /02

    36

    .46

    53

    .48

    13

    20

    0R

    57

    2

    10

    1B

    akK

    and

    i3

    42

    23

    6.4

    49

    .57

    36

    20

    0S

    30

    8

    10

    2Q

    azv

    in1

    34

    23

    36

    .26

    50

    .00

    52

    17

    4S

    45

    6

    10

    3K

    ahak

    34

    24

    36

    .12

    49

    .75

    32

    20

    0R

    *

    10

    4B

    abo

    l3

    43

    13

    6.5

    45

    2.6

    81

    41

    28

    S1

    55

    105

    Raz

    jerd

    3444

    36.3

    550.1

    85

    9154

    R898

    10

    6A

    liA

    bad

    32

    71

    /02

    36

    .90

    54

    .85

    49

    18

    R5

    62

    10

    7R

    amy

    an3

    27

    2/0

    23

    7.0

    25

    5.1

    41

    74

    2R

    82

    7

    10

    8H

    asan

    Key

    f3

    36

    5/0

    33

    6.5

    05

    1.1

    54

    12

    7S

    33

    9

    109

    Rei

    skola

    3370

    36.3

    852.0

    31

    27

    2R

    525

    11

    0N

    osh

    ahr

    33

    68

    /03

    36

    .65

    51

    .49

    15

    42

    S1

    65

    11

    1N

    oo

    r3

    36

    9/0

    43

    6.5

    75

    2.0

    11

    96

    8S

    17

    8

    11

    2N

    osh

    ahr

    31

    78

    36

    .65

    51

    .49

    15

    19

    S1

    65

    11

    3N

    oo

    r3

    41

    93

    6.5

    75

    2.0

    12

    84

    6S

    17

    8

    11

    4A

    liA

    bad

    35

    42

    36

    .90

    54

    .85

    60

    50

    R5

    62

    115

    Gonbad

    -e-K

    avoos

    3544

    37.2

    455.1

    62

    67

    8S

    402

    11

    6G

    org

    an3

    54

    53

    6.8

    45

    4.3

    91

    03

    35

    S2

    91

    11

    7G

    om

    ish

    an3

    54

    63

    7.0

    75

    4.0

    89

    14

    4S

    32

    2

    11

    8N

    eka

    35

    49

    36

    .63

    53

    .28

    23

    14

    4S

    39

    2

    11

    9R

    ezv

    an3

    55

    03

    7.1

    85

    5.7

    91

    71

    47

    S4

    94

    12

    0R

    amy

    an3

    55

    13

    7.0

    25

    5.1

    46

    17

    6R

    82

    7

    Nat Hazards

    123

  • Ta

    ble

    7co

    nti

    nued

    Nu

    mb

    er.

    Sta

    tio

    nn

    ame

    Cod

    eC

    oo

    rdin

    ate

    C.P

    GA

    a(c

    m/s

    /s)

    Hy

    po

    centr

    ald

    ista

    nce

    Sit

    ebV

    S30

    ne

    12

    1N

    oza

    rA

    bad

    35

    52

    36

    .80

    53

    .25

    47

    14

    0S

    43

    8

    12

    2A

    gh

    Gh

    ala

    35

    56

    /01

    37

    .01

    54

    .46

    69

    15

    S3

    41

    12

    3B

    and

    ar-e

    -Gaz

    35

    57

    /02

    36

    .76

    53

    .95

    67

    71

    S3

    47

    12

    4E

    stal

    kh

    Po

    sht

    35

    59

    36

    .46

    53

    .48

    50

    13

    3R

    57

    2

    12

    5D

    ibaj

    35

    90

    36

    .43

    54

    .23

    27

    83

    R5

    26

    12

    6M

    oje

    n3

    62

    2/0

    13

    6.4

    85

    4.6

    51

    67

    6R

    87

    6

    12

    7Q

    apan

    -e-O

    lya

    36

    36

    /01

    37

    .62

    55

    .68

    15

    14

    5S

    41

    0

    12

    8M

    ino

    odas

    ht

    36

    39

    /01

    37

    .23

    55

    .37

    36

    10

    1S

    44

    9

    12

    9G

    hal

    eS

    hok

    at3

    86

    23

    6.3

    55

    4.9

    12

    11

    01

    R6

    58

    13

    0A

    gh

    Gh

    ala

    35

    56

    /02

    37

    .01

    54

    .46

    18

    23

    S3

    41

    13

    1G

    om

    ish

    an3

    56

    83

    7.0

    75

    4.0

    81

    44

    9S

    32

    2

    13

    2G

    om

    ish

    an3

    60

    73

    7.0

    75

    4.0

    89

    46

    7S

    32

    2

    13

    3B

    and

    ar-e

    -Gaz

    36

    09

    36

    .76

    53

    .95

    47

    10

    1S

    34

    7

    13

    4N

    oza

    rA

    bad

    36

    11

    36

    .80

    53

    .25

    27

    16

    0S

    43

    8

    13

    5A

    liA

    bad

    36

    12

    36

    .90

    54

    .85

    34

    71

    R5

    62

    136

    Gonbad

    -e-K

    avoos

    3614

    37.2

    455.1

    61

    97

    5S

    402

    13

    7In

    cheh

    Boru

    n3

    61

    83

    7.4

    65

    4.7

    21

    63

    22

    S2

    83

    138

    Kal

    aleh

    3619/0

    237.3

    855.5

    01

    8108

    S375

    13

    9R

    amy

    an3

    62

    1/0

    23

    7.0

    25

    5.1

    44

    08

    4R

    82

    7

    14

    0M

    oje

    n3

    62

    2/0

    23

    6.4

    85

    4.6

    51

    71

    10

    R8

    76

    14

    1G

    org

    an3

    62

    33

    6.8

    45

    4.3

    86

    17

    1S

    29

    1

    14

    2D

    ibaj

    36

    24

    36

    .43

    54

    .23

    24

    11

    9R

    52

    6

    14

    3A

    gh

    ban

    d3

    63

    53

    7.6

    65

    5.1

    82

    07

    6S

    40

    2

    14

    4B

    ile-

    Sav

    ar4

    41

    73

    9.3

    64

    8.3

    23

    17

    1R

    53

    3

    Nat Hazards

    123

  • Ta

    ble

    7co

    nti

    nued

    Nu

    mb

    er.

    Sta

    tio

    nn

    ame

    Cod

    eC

    oo

    rdin

    ate

    C.P

    GA

    a(c

    m/s

    /s)

    Hy

    po

    centr

    ald

    ista

    nce

    Sit

    ebV

    S30

    ne

    14

    5H

    elab

    ad4

    41

    93

    7.9

    44

    8.4

    22

    59

    7S

    38

    7

    14

    6O

    dlo

    o4

    42

    23

    9.3

    04

    8.1

    62

    47

    5S

    44

    5

    147

    Tal

    eb-e

    -Qes

    hla

    qi

    4424

    38.4

    048.2

    12

    36

    1R

    978

    14

    8R

    azi

    44

    23

    38

    .63

    48

    .10

    21

    59

    R7

    20

    149

    Esl

    am-A

    bad

    4426

    38.1

    347.9

    41

    8104

    R1,3

    26

    15

    0L

    ahro

    od

    44

    25

    38

    .51

    47

    .83

    14

    92

    R9

    81

    15

    1N

    amin

    44

    21

    38

    .42

    48

    .48

    15

    43

    R1

    ,236

    15

    2S

    aeen

    gh

    ale

    46

    01

    36

    .31

    49

    .07

    19

    47

    R6

    42

    15

    3S

    olt

    aniy

    eh4

    60

    23

    6.4

    44

    8.8

    05

    71

    7S

    46

    6

    15

    4D

    arse

    jin

    46

    06

    36

    .02

    49

    .24

    16

    82

    R6

    36

    15

    5S

    ird

    an4

    60

    73

    6.6

    54

    9.1

    98

    35

    0S

    35

    2

    15

    6K

    ash

    mar

    46

    14

    35

    .24

    58

    .47

    15

    32

    S3

    25

    15

    7R

    ivas

    h4

    61

    53

    5.4

    85

    8.4

    64

    21

    5R

    52

    0

    15

    8C

    hen

    ar4

    71

    03

    5.2

    85

    8.9

    11

    54

    2R

    94

    0

    15

    9Y

    ekan

    kah

    riz

    46

    61

    38

    .67

    45

    .40

    29

    46

    R7

    38

    16

    0M

    aran

    d4

    66

    33

    8.4

    44

    5.7

    73

    72

    7R

    54

    6

    16

    1S

    hab

    esta

    r4

    66

    43

    8.1

    84

    5.7

    11

    35

    7R

    92

    2

    16

    2T

    aso

    oj

    46

    65

    38

    .31

    45

    .36

    14

    65

    R7

    09

    16

    3Z

    anji

    reh

    46

    66

    38

    .46

    45

    .37

    14

    56

    R9

    19

    aC

    .PG

    Aco

    rrec

    ted

    pea

    kg

    rou

    nd

    acce

    lera

    tio

    nb

    SS

    oil

    ,R

    Ro

    ck

    *B

    ased

    on

    Zar

    eet

    al.

    (19

    99)

    and

    Gh

    asem

    iet

    al.

    (20

    09b);

    atth

    ese

    site

    s,g

    ener

    icv

    alues

    of

    27

    5,

    50

    0,

    and

    1,0

    00

    m/s

    hav

    eb

    een

    assi

    gn

    edfo

    rV

    S30

    of

    clas

    ses

    III,

    II,

    and

    I,re

    spec

    tiv

    ely

    Nat Hazards

    123

  • References

    Abbassi A, Nasrabadi A, Tatar M, Yaminifard F, Abbassi M, Hatzfeld D, Priestley K (2010) Crustal velocitystructure in the southern edge of the Central Alborz (Iran). J Geodyn 49:6878

    Abrahamson N, Silva W (2008) Summary of the Abrahamson & Silva NGA ground motion relations. EarthqSpectra 24:6797

    Akkar S, Bommer JJ (2010) Empirical equations for the prediction of PGA, PGV and spectral accelerationsin Europe, the Mediterranean Region and the Middle East. Seism Res Lett 81:195206

    Akkar S, Cagnan Z (2010) A local ground-motion predictive model for Turkey, and its comparison withother regional and global ground-motion models. Bull Seismol Soc Am 100:29782995

    Ansari A, Noorzad A, Zafarani H, Vahidifard H (2010) Correction of highly noisy strong motion recordsusing a modified wavelet de-noising method. Soil Dyn Earthq Eng 30:11681181

    Ashtari M, Hatzfeld D, Kamalian N (2005) Microseismicity in the region of Tehran. Tectonophysics395:193208