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V _{S30}, slope, H _{800} and f _{0}: performance of various sitecondition proxies in reducing groundmotion aleatory variability and predicting nonlinear site response
Earth, Planets and Space volume 69, Article number: 133 (2017)
Abstract
The aim of this paper is to investigate the ability of various sitecondition proxies (SCPs) to reduce groundmotion aleatory variability and evaluate how SCPs capture nonlinearity site effects. The SCPs used here are timeaveraged shearwave velocity in the top 30 m (V _{S30}), the topographical slope (slope), the fundamental resonance frequency (f _{0}) and the depth beyond which V _{s} exceeds 800 m/s (H _{800}). We considered first the performance of each SCP taken alone and then the combined performance of the 6 SCP pairs [V _{S30}–f _{0}], [V _{S30}–H _{800}], [f _{0}–slope], [H _{800}–slope], [V _{S30}–slope] and [f _{0}–H _{800}]. This analysis is performed using a neural network approach including a random effect applied on a KiKnet subset for derivation of groundmotion prediction equations setting the relationship between various groundmotion parameters such as peak ground acceleration, peak ground velocity and pseudospectral acceleration PSA (T), and M _{w}, R _{JB}, focal depth and SCPs. While the choice of SCP is found to have almost no impact on the median groundmotion prediction, it does impact the level of aleatory uncertainty. V _{S30} is found to perform the best of single proxies at short periods (T < 0.6 s), while f _{0} and H _{800} perform better at longer periods; considering SCP pairs leads to significant improvements, with particular emphasis on [V _{S30}–H _{800}] and [f _{0}–slope] pairs. The results also indicate significant nonlinearity on the site terms for soft sites and that the most relevant loading parameter for characterising nonlinear site response is the “stiff” spectral ordinate at the considered period.
Introduction
Probabilistic seismic hazard analysis (PSHA) strongly relies on groundmotion prediction equations (GMPEs) that quantify the amplitude of ground motion as a function of distance, magnitude and sitecondition proxies (SCPs). The latter are introduced to characterise the amplification effects linked to nearsurface deposits. Given the variety of physical phenomena impacting the characteristics of an earthquake shaking, groundmotion models include a large degree of uncertainty. This uncertainty (especially the withinevent aleatory variability) is strongly affected by nearsurface site conditions. An important question is the degree to which this scatter can be reduced by improvements in the way to account for the nearsurface effects. The incorporation of those effects in GMPEs has gone through an evolution in the past years (Chiou and Youngs 2008; Seyhan et al. 2014; Derras et al. 2016). At the beginning, groundmotion models typically contained a scaling parameter based on site classification (e.g. Boore et al. 1993) or presented different models for “hard rock” and “soil” sites (e.g. Campbell 1993; Sadigh et al. 1997). Boore et al. (1997) introduced the explicit use of the timeaveraged shearwave velocity in the top 30 m (V _{S30}). V _{S30} has become de facto a standard for the development of GMPEs and seismic hazard assessment at national and international scales. In this way, it has been observed (e.g. Borcherdt 1994) that V _{S30} is a useful parameter to predict local site amplification in active tectonic regimes, especially when it is actually measured: Derras et al. (2016) showed after Chiou and Young (2008) that measuring V _{S30} allows a significant reduction in the aleatory variability.
V _{S30} has certainly proved to constitute a simple and efficient SCP metric, but it also proved not to be a lowcost SCP, as it is far from being measured at all strongmotion sites throughout the world (except in Japan). For this reason, Wald and Allen (2007) and Allen and Wald (2009) have proposed to use the topographical slope (slope) from digital elevation models (DEMs) derived from remote sensing (satellite imaging) to give a firstorder estimation of site classes based on V _{S30}. Many other ways to infer V _{S30} values without measuring them have been proposed, as listed in Seyhan et al. (2014): extrapolation from V _{S} measurements at depths shallower than 30 m, correlations—more or less robust—with other types of information or parameters (geology, geomorphological or terrainrelated proxies, geotechnical parameters).
On the other hand, V _{S30} alone cannot satisfactorily predict the amplification for sites underlain by deep sediments, which require knowledge of the geology to depths greater than 30 m (e.g. Choi and Stewart 2005; Luzi et al. 2011). Campbell (1989) found that adding a parameter for depth to basement rock improved the predictive ability of empirical groundmotion models. On their side, Cadet et al. (2011) and Derras et al. (2012) used another SCP: the fundamental resonance frequency, f _{0}, as determined by the horizontaltovertical (H/V) spectral ratio technique (Mucciarelli 1998; Haghshenas et al. 2008; Bard et al. 2010). As the f _{0} (H/V) SCP is able to identify lowfrequency amplification on thick sites, its relevance may be compared with the performance of another SCP often proposed to properly account for the sediment thickness, H _{800} (depth beyond which the shearwave velocity exceeds 800 m/s).
The main aim of this work was to assess the actual performance of several sitecondition proxies, namely V _{S30}, slope, f _{0} (H/V) and H _{800} SCP, by analysing the relative decrease in the groundmotion aleatory variability each of them allow to achieve and by investigating the benefits of considering simultaneously multiple site proxies. In addition, as all the considered ANN models were found to predict a significantly nonlinear site response, a secondary aim has been to investigate to which extent these SCPs allow to capture not only the linear, but also the nonlinear nature of site response, in combination with various loading parameters (PGA on rock, acceleration response spectrum at the period of interest PSA (T), or a siterelated strain proxy PGV/V _{S30}.
The KiKnet database used here consists of shallow crustal events recorded on sites for which several site proxies are already available: V _{S30} and H _{800} values can be directly derived from downhole measurements of V _{S} profile (Dawood et al. 2014), the slope values have been compiled (Ancheta et al. 2014), and f _{0} values are taken from Régnier et al. (2013). The KiKnet data offer the unique opportunity to have, for each strongmotion recording, a reliable measurement of the four SCPs, thus allowing a thorough and meaningful comparative assessment of the performance of each of these proxies.
The artificial neural network (ANN) approach and a randomeffectlike procedure (Derras et al. 2014) have been used for the derivation of GMPEs setting the relationship between various groundmotion parameters [peak ground acceleration (PGA), peak ground velocity (PGV) and 5% damped pseudospectral acceleration (PSA) from 0.01 to 4 s] and event/station metaparameters (moment magnitude M _{w}, Joyner and Boore distance R _{JB}, focal depth and sitecondition proxies V _{S30}, slope, H _{800} and f _{0}).
After a short presentation of the data set, a section is dedicated to the presentation of the ANN models and their specific implementation for deriving GMPEs. The following section presents the results obtained for the KiKnet data, focusing on (a) the respective performance of each of the four site proxies which are considered either alone or within combinations and (b) a discussion of their ability to detect and account for nonlinear site response.
Data set
The Kiban–Kyoshin network (KiKnet) is one of the two national strongmotion seismograph networks developed in Japan following the 1995 Kobe earthquake. The KiKnet is a network of strongmotion instruments that consist of about 700 stations with an average spacing of about 20 km distributed throughout the Japanese islands (Hayashida and Tajima 2007). The KiKnet stations are each equipped with a pair of surface and downhole, sensitive threecomponent digital accelerometers, allowing an empirical evaluation of the site response at each station.
The resulting data set considered here has been compiled by Dawood et al. (2014, 2016). This data set has been downloaded from https://datacenterhub.org/resources/272. The corresponding data processing is fully described in Dawood et al. (2014, 2016). In short, this data processing includes several steps: baseline correction, tapering on both ends (total length of tapering = 5% of the total record length), zero padding before and after recommended by Boore (2005) in relation to the order and frequency of the highpass filtering, fourthorder acausal Butterworth filtering with selection of the cutoff frequency f_{c} so that the computed final velocity and displacement values at the end of the time series remain smaller than some magnitudedependent thresholds, signaltonoise ratio larger than 3 between 2 f_{c} and 30 Hz.
The data set using here contains 977 recordings from 199 sites to 214 earthquakes. The range of M _{w}, R _{JB}, depth and all SCPs is listed in Table 1, which also provides the number of earthquakes, records and sites. The corresponding range of recorded PGA values spans from 2.6 × 10^{−4} to 0.41 g.
Sitecondition proxies
The chosen site proxies are V _{S30} and slope, which are generally considered a priori as more relevant for shortperiod ground motions, and f _{0} (H/V) and H _{800}, that should in principle be more suitable for long periods. There actually exist several possibilities proposed by different authors for such a sediment thickness parameter. It is true that most recent NGAWest and NGAWest 2 GMPEs use depths corresponding to larger velocities, as indicated by the reviewer. We have chosen to select H _{800} as a thickness parameter for the following reasons:

The database used in this study provides only the H _{800} values. H _{2500} and H _{1100} values are not available yet in this database.

The ongoing revision of European building codes recommends the use of both V _{S30} and H _{800} for site classification, since the “rock” sites are conventionally associated with V _{S30} values exceeding 800 m/s. Results associated with H _{800} are then of interest of many colleagues.
The larger the target velocity, the larger the uncertainty on the corresponding depth: even in very wellknown areas such as California, the different existing models lead to highly variable H _{2500} values (see Figure 10 in Seyhan et al. 2014). H _{800} thus seems an acceptable compromise, especially as we do not look for “basin” effects (i.e. including 2D or 3D verylowfrequency effects, such as those existing in the Los Angeles area or Kanto plain), but simply for a parameter that helps to constrain the intermediate response (around 1 s).
Groundmotion models are derived first using one single SCP [one model with each of the four values: V _{S30} or slope or f _{0} or H _{800}] and then using two SCPs out of the four [i.e. six models in total with the six pairs (V _{S30}, slope), (V _{S30}, H _{800}), (V _{S30}, f _{0}), (H _{800}, slope), (f _{0}, H _{800}) and (slope, f _{0})]. All SCPs are considered through their log_{10} values. In addition, two reference groundmotion models are established for comparison with each of the 10 previous ones: the first one is without any site proxy (named “without site proxy”), and the second one considers simultaneously all four site proxies (named “all proxies”) to estimate the maximum possible standard deviation reduction.
Data distribution
The distribution of the data set according to M _{w}, R _{JB}, focal depth, PGA and sitecondition proxy (SCP) is displayed in Figs. 1 and 2.
Figure 1 shows the distributions of the KiKnet data set in the magnitude–distance plane by bins of PGA and in the PGA–distance plane by bins of M _{w}. The distributions are given for all site conditions (left column), but also for soft sites only (V _{S30} < 300 m/s, middle column) and stiff sites only (V _{S30} > 800 m/s, right column). The goal of these presentations by bins of M _{w}, PGA and V _{S30} is to ensure that the data distribution is appropriate for all M _{w}–PGA and for soft and stiff soils. This figure also illustrates clearly the much smaller number of recordings at distances less than 10 km in general and less than 30 km when only stifftorock sites are considered.
Figure 2 represents the cumulative distribution function (CDF) of the used data set versus R _{JB}, M _{w}, V _{S30}, topographical slope, H _{800}, f _{0}, focal depth and PGA. The four SCP distributions are found to follow a lognormal distribution as well as R _{JB} and PGA, while M _{w} and focal depth are much closer to a normal distribution (see also Figure 2 in Derras et al. 2016). In our ANN models, we thus used the logarithm (base 10) values of all SCPs and spectral ordinates PSAs. Table 2 details a fractile values for each of these metadata parameters: median value, 5 and 95% fractiles which are considered to provide the range of applicability of the models, and the 10 and 90% fractiles which will be used in the following to estimate the impact of each SCP on the site amplification factor.
To ensure that the SCPs are not strongly dependent on one another, correlation plots are displayed for each pair of SCPs (Fig. 3) together with the corresponding correlation coefficient (R). Although some pairs do exhibit some correlation (R _{max} = 0.55 between V _{S30} and f _{0}), the scatter is large enough for the SCPs to be considered as almost independent site parameters for the derived ANN models. The weakest correlation is found between slope and either H _{800} or f _{0}. One may notice that H _{800} is negatively correlated with the three other SCPs: the larger it is, the lower are f _{0}, V _{S30} and slope—as could be intuitively expected. In the same figure are also indicated the median values and the 10 and 90% fractiles for the all SCPs.
Methods
The randomeffect regression algorithm made popular within engineering seismology by Abrahamson and Youngs (1992), which is arguably the most commonly used approach for developing empirical groundmotion models. In our ANN models, we used this type of approach in order to facilitate the comparability with classical GMPEs. The ANN has the advantage that no prior functional form is needed (Derras et al. 2012): the actual dependence is established directly from the data and can therefore be used as a guide for a better understanding of the factors which control ground motions. This resulted in a twophase building process.
Fixed models
The architecture of ANN used in this work is named “feedforward network”, consisting of a series of layers. The first layer ensures the connection with the input parameters, i.e. in our case M _{w}, R _{JB} and depth and one or two (or possibly more) continuous parameter describing the SCPs (V _{S30}, slope, f _{0}, H _{800}). Each subsequent layer has a connection from the previous layer. The final layer produces the network’s output. A feedforward network with one hidden layer and three neurons in the hidden layer is adopted in this study. This small number of hidden neurons is the optimal number in order to optimise both the total standard deviation of residuals σ and the Akaike information criterion (Akaike 1973). Figure 4 illustrates a typical architecture of the ANNfixed models which were implemented within the MATLAB^{®} Neural Network Toolbox™ (Demuth et al. 2009). The output layer groups all the considered groundmotion parameters, i.e. the classical geometric mean of the horizontal components of PGA, PGV and 5%damped PSA at 18 periods from 0.01 to 4 s. We did not include predictions for peak ground displacement (PGD), which we consider to be too sensitive to the highpass filters used in the data processing.
QuasiNewton backpropagation technique also called “BFGS” (Broyden–Fletcher–Goldfarb–Shanno) has been applied for the training phase (Shanno and Kettler 1970). To avoid “overfitting” problems, we chose an adequate regularisation method involving the modification of the conventional mean sum of the squares of the network errors by the addition of a term equal to the sum of the squares of the network synaptic weights and bias (Derras et al. 2012, 2014). Moreover, the optimal activation functions were found to be a “tangent sigmoïd” for the hidden layer and “linear” for the output layer.
Fully datadriven GMPEs were developed, differing by the nature of parameters used in the input layer. The first ANN model is built on the basis of the M _{w}, R _{JB} and focal depth as inputs: it accounts only for source and path effects and sets the reference to quantify the gains achieved by the consideration of the various site proxies in the other ANN models. The second pack of four ANN models considers only one SCP in the input layer, namely V _{S30}, slope, H _{800} and f _{0} (proxy1_{site} in Fig. 4). The next six ANN models investigate the combined influence of pairs of SCPs (proxy1_{site} and proxy2_{site} in Fig. 4). Finally, another set of four ANN models combining three SCPs as input parameters and one ANN model accounting simultaneously for the four SCPs are developed to provide an estimate of the maximum improvement (i.e. reduction in the standard deviation of residuals), which may be reached with the four considered site proxies.
Randomeffect model
A procedure similar to the randomeffect approach was then used to provide the between and withinevent sigma, as described in Derras et al. (2014). For each of all the considered cases, the final ANN model is obtained using the maximum likelihood approach developed by Brillinger and Preisler (1985) and stabilised by Abrahamson and Youngs (1992). The performance of the ANN scheme is measured by the σ value classically used in GMPEs, which is decomposed into the betweenevent (τ) and withinevent (ϕ) variabilities: both are zeromean, independent, normally distributed random variables with standard deviations τ and ϕ (Al Atik et al. 2010). The between and withinevent residuals are assumed uncorrelated, so that the total σ at a period T of the groundmotion model can be calculated according to Eq. 1.
Results
Performance of SCPs in reducing the aleatory variability
In this section, we compare the various models derived for KiKnet data set and analyse how the various SCPs reduce the groundmotion aleatory variability. The variations of τ, ϕ and σ versus period are displayed in Fig. 5 for all ANN models: without SCPs, one SCP and two SCPs.
Figure 5 shows that the betweenevent variability (τ) is much lower than the withinevent variability (ϕ), which is consistent with the vast majority of previous GMPE models results. The total variability (σ) is found identical at very short period (T < 0.05 s) whatever the ANN model: none of the SCP is really efficient at high frequency. The various variability components then increase from 0.05 to about 0.15 s and then decrease significantly as period is increasing. A peak around 0.1 s has already been observed by some NGAWest2 GMPEs developers (e.g. Chiou and Youngs 2014; Derras et al. 2016). A possible explanation is the interaction of varying stress drop with the highfrequency damping term (kappa). At shorttointermediate periods, i.e. for T between 0.1 and 0.6 s, oneSCP models allow reducing the withinevent standard deviation compared to the reference model. The smallest ϕ is obtained for the V _{S30} SCP, followed by f _{0} and H _{800} proxies, which have comparable performance, while the slope proxy exhibits the poorest performance. At longer periods, f _{0} and H _{800} provide the lowest ϕ values and perform better than V _{S30}.
As expected, the twoSCP models lead to larger variance reductions, but it is interesting to notice than all pairs of proxies exhibit very similar performance. At shorttointermediate periods, i.e. from 0.4 to 0.8 s, the [V _{S30}, f _{0}] pair is found to provide the smallest values of ϕ, while for T > 0.8 s the “best” pair turns out to be [f _{0}, H _{800}] as logically expected since both parameters are more sensitive to the bedrock depth. Interestingly enough, the [f _{0}, slope] pair exhibits a relatively good performance over the whole period range [0.1–4 s], while it is associated with the lowest measurement cost.
In addition, to better quantify the gains achieved by each SCP (s) model, the values of the variance reduction coefficients R _{ σ }, R _{ ϕ } and R _{ τ } defined in Eq. 2 are presented in Fig. 6. The variations of these coefficients versus period are displayed in Fig. 6 for all ANN models: without SCPs, oneSCP, twoSCP, the best threeSCP model and the single fourSCP models. The reason for which we add these three and four SCPs cases is to obtain an estimate of the maximum possible variance reduction when many site parameters are known. The R _{ σ } values are also listed in Table 3 for a limited set of groundmotion parameters (PGA, PGV and PSA at T = [0.2, 0.5, 1.0, 2.0] s).
The obtained results confirm that the reduction in the aleatory variability becomes significant beyond T = 0.1 s and for PGV as well (Table 3). For the short periods [0.1–0.6 s], the best is V _{S30}—with a maximum of 25% variance reduction at 0.4 s—while f _{0} outperform in the [0.6, 4] s. The variance reduction obtained with the slope SCP is the lowest of all SCPs (except between 0.1 and 0.2 s) and reaches a maximum of 9% at 4 s. V _{S30} is thus confirmed to be relevant mainly for shorttointermediate periods, as expected from the fact that it samples only the shallow subsurface, while f _{0} and H _{800} are more sensitive to the deep sediments and more relevant for long periods. Similarly, the “twoSCP” models exhibit a slightly larger variance reduction at shorttointermediate period when they include V _{S30} as one of the two site proxies (the best performance being achieved by the [V _{S30}, f _{0}] pair), while the largest reduction at long periods is observed for the [f _{0}, H _{800}] pair, i.e. a combination of two longperiod proxies, with a value of R _{ σ } reaching 24% at T = 2.0 s. Overall, the largest reduction is observed for the “reference” model accounting simultaneously for the four SCPs, followed by the three best SCPs model combining the use of [V _{S30}, f _{0}, H _{800}]; it is noteworthy, however, that such “maximum possible” variance reduction does not exceed 1.5% for PGA (Table 3) and 4% for short periods around 0.08 s, while it reaches 29% around 0.4 s. The values of these variance reduction coefficients confirm that no site proxy can be preferred over the whole frequency range.
It is worth noticing in Figs. 5 and 6 that site proxies also influence the betweenevent standard deviation τ in a very similar way they affect the withinevent variability: it could be interpreted as resulting from the fact that a better site description enables a better description of the actual dependence of the dependence on the source and path parameters. It may also indicate that despite the randomeffect procedure, the within and betweenevent variabilities are not completely independent. Such dependency with a slight tradeoff between source and siterelated residuals has already been observed and cannot be avoided (e.g. Ktenidou et al. 2017).
Another parameter used in ANN approach to measure the relevancy of each explanatory variable (and therefore of each single SCP or SCP pair) is the total percentage of synaptic weights P. As explained in Derras et al. (2012) and Derras et al. (2014), these synaptic weights P can be estimated from the weights allocated to each input variable in each connection to the hidden layer and provide a measure of the relative, overall importance of the individual explanatory variables, averaged for all the output groundmotion parameters (thus, here, over the whole frequency range 0.01–4 s). They have been computed according to the procedure detailed in Derras et al. (2014, Equation 4), for the 11 ANN models. Tables 4 and 5 list the P values (in %) for each input variable. As expected from the data distribution, the most efficient parameter in reducing the variance of response spectra is the R _{JB} distance (synaptic weight around 40–51%), followed directly by the earthquake magnitude M _{w} (around 27–36%). The P values associated with the site term range from 7 to 31%. However, focal depth does not have a great importance (P _{Depth} ≅ 6).
When only one SCP is considered, the largest SCP weights correspond to V _{S30} (around 19%) and H _{800}(≅ 18%), while the smallest corresponds to the slope (P _{slope} = 7%). For the twinSCP models, the best pair is (V _{S30}, H _{800}) with P = 25%. The [f _{0}, slope] pair also performs well with P = 21%. This ranking is similar to the ranking obtained from the analysis of aleatory variabilities discussed above if we consider the whole period range.
As in the aleatory variability analysis described above, the “all proxies” model is considered for comparison. The total synaptic weight of SCPs reaches 31%, which decomposes in individual synaptic weights for each SCP ranking as for the synaptic weight of oneSCP models: the largest one is \( P_{{V_{{{\text{S}}30}} }} \), followed by \( P_{{f_{0} }} \) and \( P_{{H_{800} }} \), the poorest one is associated with the slope (P _{Slope} = 3%). When the number of SCP increases, the increase in the SCP weight is associated first with a decrease in the magnitude and R _{JB} weights (from one SCP to two SCPs), while the relative importance of the focal depth (from two SCPs to four SCPs) is 5–6%: the importance of focal depth is not affected by the site described, while R _{JB} and M _{w} obviously remain key parameters.
Impact of the various SCPs on median groundmotion models
As discussed above, the nature of SCP has a noticeable effect on the groundmotion aleatory variability. We investigate here their impact on the median estimates, through a comparison of the four oneSCP ANN and six twoSCP ANN models. Figure 7 displays the distance dependence of the spectral acceleration for T = 0.0, 0.2 and 1.0 s, for the median magnitude (M _{w} = 5.1), the median focal depth (9 km), and the median values of the various SCPs (i.e. V _{S30} = 468 m/s, f _{0} = 4.2 Hz, H _{800} = 20 m and slope = 0.045 m/m, as derived from Fig. 2 and Table 2). Through Fig. 7a, we remark that the site proxy type (V _{S30}/f _{0}/H _{800}/slope) is observed not to have any significant impact on median predictions.
The twoSCP models (Fig. 7b) lead to similar results. All pairs of proxies exhibit very similar median predictions, especially at short periods (T = 0.0 s, T = 0.2 s and T = 1.0 s). Furthermore, the comparison with the V _{S30}SCP model highlights the fact that the type and the number (one SCP or two SCPs) of site proxies have no influence on this median.
Ground motions for “Extreme” values of site proxies
Complementary information is provided by the amount of difference in predictions for “extreme” values of the SCP. Figures 8 and 9 display the “soft/stiff” spectral ratio (SR) for various periods (T = 0.0, 0.2 and 1.0 s): a consistent definition of “soft” and “stiff” sites was taken for all SCPs, simply by considering the SCP values corresponding to 10 and 90% of the CDF distributions shown in Fig. 2 and listed in Table 2; note, however, that given the negative correlation between H _{800} and other proxies, the 10% fractile of H _{800} (i.e. 4 m) has been associated with the 90% fractile of V _{S30}, f _{0} and slope (i.e. 829 m/s, 11.71 Hz and 0.117 m/m, respectively), and vice versa (i.e. 86 m, 289 m/s, 0.66 Hz and 0.015 m/m, respectively). Figures 8 and 9 display such SR for individual SCP (top) and twoSCP (bottom) cases. SR has the following form:
Figure 8 shows the sensitivity of the SR amplification factors to R _{JB} distance, at three different spectral periods (0.0, 0.2 and 1 s), and for a given earthquake scenario (M _{w} = 6, depth = 9 km). Besides the trend of site amplification to increase with distance up to 100 km—which is related to nonlinear site response as the loading level is decreasing with increasing distance—the site amplification is found to increase with period, as classically found in most GMPEs. The curves are displayed between [20 and 100] km, considered reliable, since the derived models can hardly be considered reliable for soft and stiff sites at lower distances to 20 km or greater than 100 km (see Fig. 1). V _{S30} and slope SCPs are found to provide the amplification at short periods (which remains, however, smaller than 27%). The situation is opposite at long period (T = 1.0 s) where the SCP providing the largest amplification is f _{0} with amplification ranging from 2 to 3. In addition, it is clear that the site amplification predicted with the slope proxy is not very sensitive to the oscillator period. Another interesting result is that the combination of two proxies significantly increases the “soft/stiff” SR values: the amplification increase ranges from 3% (V _{S30} to V _{S30} –slope) at short period, to 12% at intermediate periods, to 16% at long period (f _{0} to f _{0}–V _{S30}). The most probable explanation comes from the fact that simultaneously matching 10 and 90% fractiles for a pair of proxies corresponds to less frequent combinations, with more differentiated site conditions, than for a single proxy (as also shown in Fig. 3).
Figure 9 illustrates the SR amplification factors variation versus PSA_{stiff} at T = 0.0 s (i.e. PGA_{stiff}), one of the reference parameters that is commonly used in GMPEs to describe the dependence of the nonlinear site amplification on the loading level. These curves have been established here by considering a given R _{JB} distance (30 km), a given focal depth (9 km) and a magnitude varying from 5 to 7 with an equal increment 0.125. A closer look at the dependence of soft/stiff amplification factor does indicate a larger amplification level for small stiff motion levels, associated with a significant nonlinearity (i.e. decrease in amplification with increasing loading level at the underlying bedrock). The curves displayed in Fig. 9 call for several comments:

1.
The amount of nonlinearity depends both on the considered site proxies and on the oscillator period.

2.
Whatever the site proxy, a significant nonlinearity can be observed at long period (T = 1 s), which is a somewhat unexpected result.

3.
Among single proxy models, the one using the slope predicts similar nonlinearity whatever the oscillator period, while the “longperiod” proxies f _{0} and H _{800} are those who do not predict any significant nonlinearity at short period: the predicted SR is around 1 at T = 0.0 s and around 1.8 to 1.5 at T = 0.2 s. At long period (T = 1.0 s), the SCP providing the largest SR is f _{0}, while amplification levels and their nonlinear sensitivity on PGA_{stiff} are almost similar to V _{S30} and H _{800} proxies. This larger amplification factors for the f _{0} model at T = 1.0 s might be related to the fact that the “soft” site is characterised by a fundamental frequency of 0.66 Hz: the oscillator frequency (1 Hz) is always larger than the fundamental frequency, and one may thus expect to be systematically in the amplified frequency range, while sites with V _{S30} = 289 m/s or H _{800} = 86 m, with fundamental frequencies above 1 Hz (see the last column of Fig. 3), do exist. Correlatively, a larger reduction in the amplification with increasing loading level may be expected if the nonlinear behaviour affects the whole thickness of the soil deposit (see Régnier et al. 2016).

4.
Similar observations can be done for the results with twoSCP models. At short period (T = 0 and 0.2 s), the largest amplification and nonlinearity are predicted when using the pair of shortperiod proxies (V _{S30}–slope and V _{S30} –f _{0}), while the smallest corresponds to the pair of longperiod proxies (f _{0}–H _{800} and H _{800} –slope). At long period (T = 1.0 s), the predicted amplifications and their nonlinear component are less scattered than in the oneSCP case, the pairs including the f _{0} proxy predicting, however, slightly larger amplifications.
These results are, however, partial and should not be extrapolated too fast, as they correspond to a specific distance (and focal depth) and use the stiffsite PGA to characterise the loading level.
Figures 10, 11, 12 and 13 are thus intended to check the robustness of the results presented in Fig. 9, considering also other descriptions of the loading level and other distance scenario. Only oneSCP models are considered, successively V _{S30}, f _{0}, H _{800} and slope for Figs. 10, 11, 12 and 13, respectively. In each case, three different distances are considered (30, 50 and 75 km) i.e. in the range where there exist enough data within the [10–90%] fractile range of each SCP, and the variation of the loading level for each distance corresponds to the predictions over the magnitude range [5–7] with an equal increment of 0.125. Three different parameters are considered to characterise the loading level: the PGA on rock or “stiff” site as defined according to the selected site proxy, the spectral acceleration on the same rock or “stiff” site at the oscillator period considered, and finally an estimate of the actual strain at the site: several authors (Idriss, 2011; Chandra et al. 2015, 2016; Guéguen 2016) proposed to use the ratio PGV/V _{S30} as a proxy to the shear strain, where PGV is the peak velocity at the site, and it has thus been tested in the present study. In principle, if a loading parameter is relevant for nonlinear behaviour, the dependency of site amplification as a function of this loading parameter should exhibit only a marginal dependency on other parameters such as magnitude, or distance or frequency contents. Analysing Figs. 10, 11, 12 and 13 according to this criterion clearly indicates that the lowest scatter is observed among distance and magnitude scenarios for the loading parameter “PSA_{stiff}(T)” (second row), while the largest corresponds to “PGA_{stiff}”, especially for the longperiod site amplification.
In the light of these results, it turns out that the best groundmotion parameter to be used for the characterisation of the loading level in the nonlinear site amplification term of GMPEs is the spectral ordinate on rock at the considered period; the strain proxy PGV/V _{S30} may, however, constitute a satisfactory, alternative choice. Another major outcome of this section is the variability of the nonlinear behaviour according to the site proxy selected for the GMPEs: shortperiod nonlinearity is observed preferably with shortperiod proxies (V _{S30} and slope) and disappears when using H _{800}.
Summary and conclusions
The application of neural networks approach to a KiKnet data set offered the possibility to test the performance of various sitecondition proxies to reduce the aleatory variability in GMPEs. The four available SCPs are V _{S30} and H _{800} (both derived from downhole measurements), f _{0} (the fundamental frequency derived from H/V ratios and surface/downhole spectral ratios), and the slope derived from DEM data, which has been proposed as a proxy to V _{S30} values. A total of 16 neural network models were derived to describe the dependence of response spectra ordinates on moment magnitude M _{w}, Joyner and Boore distance R _{JB}, focal depth and various combinations of SCPs: one without any SCP which provides the “reference case”, four with each single SCP, six with the six possible pairs of SCPs [V _{S30} –f _{0}], [V _{S30} –H _{800}], [f _{0} –slope], [H _{800} –slope], [V _{S30} –slope] and [f _{0} –H _{800}], four with the four possible combinations of three SCPs, and one will all SCPs considered simultaneously.
When only one SCP is used, the largest reduction in aleatory variability with respect to the “reference case” is found to be provided by V _{S30} at shorttointermediate periods (T ≤ 0.6 s), and by f _{0} or H _{800} at longer periods. Among the four SCPs, the parameter “slope” is thus found to provide the worst performance when considered alone. However, when SCP pairs are considered, comparable performance is found whatever the pair of proxies. In particular, the “best pairs” are found to be [V _{S30} –H _{800}] at short periods and [f _{0} –H _{800}] at long periods, while the “lowcost” pair [f _{0} –slope] provides a good compromise over the whole period range [0.1–4 s]. None of the four tested SCPs is thus “optimal” over the whole period range, and all proxies show a poor contribution at high frequencies (>10 Hz).
Otherwise, the site proxy type (slope/V _{S30}/H _{800}/f _{0}) has no influence on the median, and these results indicate that the type of SCP does not really affect the median.
Regarding site amplification, V _{S30} and slope SCPs are found to provide some differentiation at short periods (0, 0.2 s). At long period, H _{800} and f _{0} are providing the largest differentiation. We showed also that, for this subset of KiKnet data, the softtostiffsite amplifications exhibit a significant nonlinearity, the characteristics of which are, however, tightly linked to the used proxy, and the parameter selected to describe the loading level. The most relevant loading parameter is found to be the spectral acceleration on rock (or “stiff” site) at the considered period, and the worst the rock (or “stiff”) peak acceleration, with a satisfactory behaviour for the strain proxy PGV/V _{S30}. Nonlinearities are found to be systematically larger at intermediate period (1 s) than at short period (0.2, 0 s). This purely datadriven result is rather intriguing and calls for further checks, such as the use of larger data sets, especially at long periods (for instance, adding recordings from interplate earthquakes), the comparison with the sitespecific nonlinearities as defined by the RSR_{NLL} ratio introduced by Régnier et al. (2013, 2016), i.e. the ratio between the surfacedownhole transfer function obtained for strong motion and the transfer function derived only for weak motions, and possibly the testing of other, basinrelated, site proxies such as H _{1100} or H _{2500}.
Another important result (which will also have to be investigated further) is the variability of the nonlinear site response according to the SCP: shortperiod nonlinearity is observed preferably with shortperiod proxies (V _{S30} and slope) and disappears when using H _{800}.
As these results have been obtained on a specific—though large—data set (subset of KiKnet data, thus probably lacking of very soft sites), they should of course be tested for other data sets; the four SCPs are, however, rarely available simultaneously.
Abbreviations
 SCP:

sitecondition proxy
 V _{S30} :

timeaveraged shearwave velocity in the top 30 m
 H _{800} :

depth beyond which V _{s} exceeds 800 m/s
 f _{0} :

fundamental resonance frequency
 Slope:

topographical slope
 DEM:

digital elevation models
 PGA:

peak ground acceleration
 PGV:

peak ground velocity
 PSA:

pseudospectral acceleration
 GMPEs:

groundmotion prediction equations
 ANN:

artificial neural network
 M _{w} :

moment magnitude
 R _{JB} :

Joyner and Boore distance
 Depth:

focal depth
 CDF:

cumulative distribution function
 R :

coefficient of correlation
 τ :

betweenevent standard deviation
 ϕ :

withinevent standard deviation
 σ :

total standard deviation
 R _{ τ } :

betweenevent variance reduction coefficient
 R _{ ϕ } :

withinevent variance reduction coefficient
 R _{ σ } :

total variance reduction coefficient
 P:

total percentage of synaptic weights
 SR:

spectral ratio
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Authors’ contributions
Most of the scientific and technical work has been carried out by BD, under the scientific supervision of PYB and FC. The redaction has been shared among the three authors. All authors read and approved the final manuscript.
Acknowledgements
The authors thank Julie Régnier and Héloïse Cadet for their generous help and which provided us the f _{0} of the KiKnet database. We acknowledge the support from the TASSILI program, the sinaps@ project (http://www.institutseism.fr/projets/sinaps/). We also thank an anonymous reviewer for their constructive criticism and comments that helped us to improve this study. The authors would like to thank Haitham Dawood and Adrian RodriguezMarek for providing highquality data.
Competing interests
The authors declare that they have no competing interests.
Data and resources
PSA, V _{S30} and H _{800} used in this study were collected from the KiKnet website https://datacenterhub.org/resources/272. Slope have been collected and disseminated by the “The Pacific Earthquake Engineering Research Center” at http://peer.berkeley.edu/ngawest2/databases/. f _{0} from Régnier et al. (2013).
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Derras, B., Bard, PY. & Cotton, F. V _{S30}, slope, H _{800} and f _{0}: performance of various sitecondition proxies in reducing groundmotion aleatory variability and predicting nonlinear site response. Earth Planets Space 69, 133 (2017). https://doi.org/10.1186/s406230170718z
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DOI: https://doi.org/10.1186/s406230170718z
Keywords
 Aleatory variability
 Sitecondition proxies
 KiKnet
 Neural networks
 GMPE
 Nonlinear site response