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Assessment of nonlinear site response at ocean bottom seismograph sites based on Swave horizontaltovertical spectral ratios: a study at the Sagami Bay area KNET sites in Japan
Earth, Planets and Space volume 69, Article number: 29 (2017)
Abstract
We analyzed Swave horizontaltovertical (SH/V) spectral ratios at six ocean bottom seismograph (OBS) sites of KNET located in the Sagami Bay area of Japan for nonlinear site responses. The degree of nonlinearity was computed by comparing the SH/V spectral ratios for strong motions (PGA ≥ 20 cm/s^{2}) with those for weak motions (PGA < 20 cm/s^{2}). Our analyses, which showed that the weakmotion SH/V spectral ratios differ from site to site, indicate that the underlying site geology is not uniform at the OBS sites. It was found that the threshold PGA causing a nonlinear site response is generally different from site to site. Recordings having horizontal PGAs greater than about 50–150 cm/s^{2} display clear signatures of nonlinear site effects, i.e., the shift of predominant frequencies to lower ones and/or the decrease in highfrequency spectral ratios. We also found that the degree of nonlinearity is generally larger at the OBS sites due to the smaller threshold motions that cause a nonlinear site response compared with the available data at land sites. The above findings suggest the possibility of a widespread nonlinear site response at the OBS sites for offshore earthquakes with a large magnitude. However, frequencies lower than about 2 Hz are not affected by the nonlinear site response in the analyzed data ranges (PGA < 467 cm/s^{2}). These results indicate the need for careful utilization of recorded strong motions at OBS sites for applications such as realtime ground motion predictions as front detections.
Background
Soft soil sites undergo nonlinear site responses during strong shakings. A peak ground acceleration (PGA) of 100–200 cm/s^{2} has generally been cited as a threshold motion that causes a nonlinear site response (e.g., Beresnev and Wen 1996). The classical approach compares the spectral ratios of observed recordings at a site with respect to those at a reference rock site to identify nonlinearity. A major limitation of this approach, however, is the availability of a reference rock site that is close enough to the soil site to cancel the source and propagation path effects (e.g., Field et al. 1997). In contrast, the deployment of vertical array strongmotion observations in different parts of the world provides a unique opportunity to understand linear as well as nonlinear site responses during strong shakings (e.g., Satoh et al. 1995; Wen et al. 1995; Bonilla et al. 2002; Tsuda et al. 2006). Using the surface and borehole site pairs of KiKnet stations, Wu et al. (2010) pointed out nonlinear site responses even for shakings as low as about 20–30 cm/s^{2}. The nonlinear site response is identified by the reduction in amplitude of highfrequency components and the shift of predominant frequencies to lower ones during strong motions in comparison with those during weak motions; these effects are due to the increase in damping and degradation of the shear rigidity of soils during strong shakings (e.g., Beresnev and Wen 1996).
Wen et al. (2006) proposed a single station method using the horizontaltovertical spectral ratios of Swaves (SH/V) to identify the nonlinear site effects. In this method, the mean SH/V spectral ratios for weak motions at a site are considered to be the reference spectral ratios and are compared with the SH/V spectral ratios for strong motions at the same site. Using the method of Wen et al. (2006), Noguchi and Sasatani (2008, 2011) identified the nonlinear site effects at KiKnet sites during strong shakings; it was verified that the SH/V spectral ratios of surface recordings have features similar to those depicted by the surface and borehole station pairs. The SH/V method is especially useful for sites where the station pairs or vertical array measurements are unavailable.
Deployments of largescale ocean bottom networks that comprise seismometers and pressure gauges (e.g., DONET in the Nankai Trough area, DONET 2016; Snet in the Japan Trench area, Kanazawa 2013) are expected to contribute to earthquake and tsunami early warnings by prompt detection of earthquakes at subduction zones. The amplification effects of soft sediments at the ocean bottom seismograph (OBS) sites on the overestimation of displacement–amplitudebased magnitudes have already been discussed (Hayashimoto and Hoshiba 2013; Nakamura et al. 2014). Hayashimoto et al. (2014) analyzed the SH/V spectral ratios at three off Kushiro OBS sites and showed that recordings having a PGA of about 100 cm/s^{2} or greater display the nonlinear site response. These results indicated that the reliable prediction of strong motions using the OBS sites as front stations is impossible without taking the nonlinear site effects into account. In this regard, it is important to identify nonlinear site response characteristics such as threshold PGAs, shift of predominant frequencies, and reduction in highfrequency amplifications at the OBS sites to effectively utilize the strongmotion recordings at the OBS sites for realtime applications.
Because the OBS sites are located several kilometers away from the land stations and do not have deep vertical array observations, the SH/V spectral ratio method is useful for the identification of nonlinear site responses at the OBS sites. Many weakmotion recordings and several strongmotion recordings exceeding 100 cm/s^{2} are available at each of the six Sagami Bay area OBS sites. In this paper, we apply the Swave H/V spectral ratio method to investigate the nonlinear site effects at the Sagami Bay area OBS sites, namely the KNG201, KNG202, KNG203, KNG204, KNG205, and KNG206 sites (Fig. 1). The data from these OBS sites are available as a part of the KNET observation system (Aoi 2004). The distance interval between two adjacent OBS sites is approximately 20 km, and the depths of oceanic water range between about 1000 and 2000 m. Details about the deployment of the OBS sites used in this study can be found in Eguchi et al. (1998).
Data and methodology
We used 935 threecomponent ocean bottom accelerograms from 315 earthquakes. The accelerograms have the following properties: (1) horizontal vector PGA > 5 cm/s^{2}, (2) both P and Swave onsets are included in the recordings, and (3) signaltonoise ratio is greater than 3 for each frequency component. In this paper, we define the PGA as the horizontal vector PGA obtained from two horizontal component recordings. The epicenters of the earthquakes used in this study are shown in Fig. 1. We used recordings from earthquakes having Japan Meteorological Agency magnitudes (Mj) between Mj = 3 and Mj = 7. Most of the recordings having PGAs > 20 cm/s^{2} are from earthquakes between Mj = 4.0 and Mj = 6.6. An example of recordings with preevent noise, Swave time windows, and their Fourier amplitude spectra is shown in Additional file 1. The epicentral distance was arbitrarily restricted to 200 km for recordings having PGA < 20 cm/s^{2} to reduce the data processing time because a large number of recordings are available for smaller motions and to 300 km for recordings having PGA ≥ 20 cm/s^{2} to increase the number of such strongmotion recordings. The focal depths of the earthquakes were shallower than 150 km.
Wu et al. (2010) noted a time window of 6 s as a balance between the stability of the computed spectra and the temporal changes for recordings from earthquakes with relatively smaller magnitudes. In this study, we used a time window of 10 s starting from 1 s before the Swave onset considering the stability of the computed spectra as temporal changes were not investigated. We picked the Swave onset manually, and halfcosine tapering was applied for 1 s at both ends of the time window. The time window was extended to 40.96 s by padding zeroes to compute the Fourier spectral amplitudes. The horizontal spectral amplitudes were derived as the vector sum of two horizontal components, and both horizontal and vertical spectral amplitudes were smoothed by applying a Parzen window of 0.4 Hz. Then, SH/V spectral ratios were obtained.
We adopted the equation (Eq. 1) proposed by Noguchi and Sasatani (2008) to quantify the degree of nonlinearity (DNL) based on the SH/V spectral ratios. The equation is shown below.
where R _{strong} and R _{weak} represent the SH/V spectral ratios for strong motions and weak motions, respectively, and ∆f is the frequency interval. One of the advantages of this DNL index is that it gives a single value that facilitates the comparison with other parameters such as the PGA. We calculated the DNL from spectral ratios between 0.5 Hz and 20 Hz. An example plot of SH/V spectral ratios from two groups of recordings, PGA < 20 cm/s^{2} and 20 cm/s^{2} ≤ PGA ≤ 50 cm/s^{2}, is shown in Additional file 2 for the KNG201 site. We found that the mean spectral ratios for the two groups of recordings are nearly identical. We adopted the mean spectral ratios from recordings having PGA < 20 cm/s^{2} as R _{weak} and spectral ratios from recordings having PGA ≥ 20 cm/s^{2} as R _{strong} for all sites. Noguchi and Sasatani (2011) suggested a DNL value of 4 to identify the nonlinear site response in consideration of the stability of the SH/V spectral ratios for individual recordings. Our preliminary results (Dhakal et al. 2016) support that this value of DNL is reasonable to identify the nonlinear site response when using the same processing techniques of Noguchi and Sasatani (2011) to derive the spectral ratios. A comparison of the weakmotion mean SH/V spectral ratios (R _{weak}) at the six OBS sites is shown in Fig. 2. The R _{weak} values, computed from 60 to 115 recordings (earthquakes) at each site (see Additional file 2, for an example), show that the peak frequencies are different from site to site. This difference suggests that the local geology is generally different from site to site (e.g., Kawase et al. 2011), and the degree of nonlinear site response is also expected to be different at each site, as described in the next section.
Results and discussion
We obtained the DNL at each of the OBS sites by using the methodology described in the previous section. We show a comparison of the SH/V spectral ratios of the weak motion with those of the strong motion at the KNG201 and KNG203 sites in Fig. 3a, b, respectively, for selected recordings having PGA > 100 cm/s^{2}. The DNL values are also shown for each recording. Similar comparisons at the KNG202, KNG204, KNG205, and KNG206 sites are provided in Additional file 3. Here, the KNG201 and KNG203 sites are selected to illustrate how closely the DNL values and other features such as the shift of periods and the decrease in highfrequency components change with shaking levels. Also, the KNG201 and KNG203 sites have SH/V spectral ratios of the weakmotion peak at somewhat separated frequencies, as shown in Fig. 2. Thus, the comparison clarifies the site response behavior between two different site conditions. Figure 3a shows the comparison of SH/V spectral ratios for four recordings having PGAs 123, 124, 192, and 247 cm/s^{2} at the KNG201 site. SH/V spectral ratios of the weak motion show a broader peak from 1 to 2 Hz at the KNG201 site. No clear shift of peak frequency and systematic reduction in highfrequency spectral ratios can be identified at the KNG201 site for the four strongmotion recordings mentioned above. For the first two recordings having PGAs 123 and 124 cm/s^{2}, the DNL values are smaller than 4. For the other two recordings having PGAs 192 and 247 cm/s^{2}, the DNL values are 4.2 and 4.9, respectively. However, a close examination of the spectral ratios for the 247 cm/s^{2} recording shows an opposite trend of the spectral ratios at a frequency of about 20 Hz. This trend suggests that the DNL value for this recording is exaggerated. In summary, the KNG201 site has a small nonlinear site response even for a PGA of about 200 cm/s^{2}.
A comparison of the SH/V spectral ratios at the KNG203 site for four recordings having PGAs 150, 175, 202, and 284 cm/s^{2} is shown in Fig. 3b. SH/V spectral ratios of the weak motion at the site show peak frequencies between 5 and 10 Hz. Unlike the KNG201 site, a clear decrease in highfrequency spectral ratios between 7 and 20 Hz can be seen for all of the PGAs mentioned above, and the clear shift of peak frequencies to lower ones can be identified for the two largest PGAs. The computed DNL values are greater than 7.5 and agree with the visual comparisons from which substantial nonlinearity can be stipulated. It is noted that the largest PGA in the analyzed data is 467 cm/s^{2} recorded at the KNG205 site; the DNL value is 7.3; and a clear shift of peak frequency and reduction in highfrequency spectral ratios can be identified (see Additional file 3). Our analysis indicated that the spectral ratios at frequencies lower than 2 Hz are not affected by the nonlinear site response in the analyzed data ranges.
The relationship between the PGAs and DNL values is summarized in Fig. 4a–f for the six OBS sites. The flattened trend of the DNL values at lower PGAs indicates that the site response is linear for these recordings. At the KNG201, KNG202, and KNG206 sites, the DNL values are less than 4 for PGAs less than about 150 cm/s^{2} and then increase almost similarly with the increase in PGAs. At the KNG203 site, the DNL values are larger than 4 for PGAs larger than about 50 cm/s^{2} and increase linearly with the increase in PGAs. Because the nonlinearity appears at relatively lower PGAs at the KNG203 site, the flattened trend of the DNL values cannot be recognized well between 20 and 50 cm/s^{2}. Therefore, at the KNG203 site, we added the DNL values computed for 10 cm/s^{2} to less than 20 cm/s^{2} recordings with respect to the mean spectral ratios computed from 39 recordings having PGAs between 5 cm/s^{2} and less than 10 cm/s^{2}. The added data helped to clearly see the flattened trend of the DNL values at PGAs less than about 40 cm/s^{2} (see Fig. 4c) and indicate a linear response at lower PGAs. Because the mean spectral ratios for weak motions in the two groups, 5–10 cm/s^{2} and 10 to 20 cm/s^{2}, are found to be essentially identical, the DNL values for recordings having PGAs ≥ 20 cm/s^{2} are not discussed further with respect to the mean spectral ratios for 5–10 cm/s^{2} recordings. At the KNG204 site, the DNL values are less than 4 for PGAs less than about 100 cm/s^{2} and rise sharply at PGAs of about 150 cm/s^{2}. The KNG205 site shows larger variability for smaller PGAs less than about 100 cm/s^{2}, with DNL values occasionally rising over 4. On average, the DNL value is smaller than 4 for PGAs less than about 200 cm/s^{2} and larger than 4 for PGAs larger than about 200 cm/s^{2} at the KNG205 site. The relationship between the DNL values and PGAs suggests that the sites behave nonlinearly only after reaching the threshold PGA, which generally varies from site to site. These results are consistent with the fact that the soil response is linear at small strain levels and behaves nonlinearly at large strains.
As we applied the same processing technique as Noguchi and Sasatani (2011), it is interesting to see how the DNL values obtained at the OBS sites and those obtained at the land sites by Noguchi and Sasatani (2011) are different with respect to the values of PGAs. The results from the present study and those from Table 1 of Noguchi and Sasatani (2011) are compared in Additional file 4. We found that the DNL values at the land sites and four OBS sites, namely KNG201, KNG202, KNG205, and KNG206, change almost similarly with the comparable PGAs. However, at two OBS sites, KNG203 and KNG204, the DNL values for PGAs of about 200 cm/s^{2} are about twice the DNL values for the corresponding PGAs at the land sites. These results are not surprising given the possibility of very soft site conditions at the OBS sites, where the nonlinear site response may begin at much lower levels of shakings. Furthermore, strong attenuation of highfrequency motions due to the soft layers at the OBS sites is possible.
Finally, we compare the peak frequencies and spectral ratios at the peak frequencies of weak motions between the weakmotion (PGA < 20 cm/s^{2}) and selected strongmotion recordings (PGA > 100 cm/s^{2}) in Fig. 5a, b, respectively. The conceptual plot shown in Fig. 5c defines the peak frequencies and spectral ratios for the comparison between the weak and strong motions. It can generally be seen that the peak frequencies of strong motions are lower than the peak frequencies of weak motions; the shift of peak frequencies occurs between about 20 and 55% depending on the site (Fig. 5a). For example, the shift of peak frequencies for strong motions can clearly be seen for the KNG204 and KNG206 sites (see also the additional files). However, it is sometimes difficult to quantify the shift of peak frequencies, even though a clear decrease in highfrequency spectral ratios can be observed (see lower panels of Fig. 3b); this is due to the relatively wide peak at some sites. Figure 5b shows a plot of spectral ratios for strong motions at the peak frequency of weak motions against the peak spectral ratios for weak motions. The tendency for reduction in the peak spectral ratios can clearly be seen at the sites where the values of the DNL are large. The reduction in spectral ratios occurs in about 5–70% of the peak spectral ratios for weak motions in the analyzed data ranges. Again, the reduction in peak spectral ratios cannot be well quantified for some recordings due to the broader peak at some of the sites. In such cases, the DNL values, however, are still large and suggest the nonlinear site response at these sites. We find that the shift of peak frequencies and reduction in peak spectral ratios are generally larger for stronger motions at the same site. These results are similar to those reported in Wu et al. (2010) for some KiKnet sites.
Conclusions
We analyzed SH/V spectral ratios for identifying the nonlinear site responses at six OBS sites of KNET located in the Sagami Bay area of Japan. SH/V spectral ratios from weak motions having PGA < 20 cm/s^{2} were used as reference spectra for each OBS site. We found that the weakmotion SH/V spectral ratios differ from site to site. The difference suggests that the local geology is not uniform beneath the recording stations. The degree of nonlinearity was computed by using the method proposed by Noguchi and Sasatani (2008, 2011) for recordings having PGA ≥ 20 cm/s^{2}. Our results showed that the SH/V spectral ratios for strongmotion recordings having horizontal PGAs greater than 50–150 cm/s^{2}, depending on the site, display signatures of a nonlinear site response at the OBS sites. That is, the shift of peak frequencies to lower ones and the decrease in highfrequency spectral ratios are well identified above the threshold PGAs, which are site dependent. We found that the degree of nonlinearity was remarkably larger at some of the OBS sites due to the smaller threshold motions to cause a nonlinear site response at the OBS sites. The lower threshold PGAs at some of the OBS sites might indicate that pervasive nonlinear site effects occur at the OBS sites during offshore earthquakes of large magnitude and greatly diminish the highfrequency components of strong motions and cause a considerable shift of peak frequencies to lower ones. These results suggest the need for careful use of the recorded strong motions at the OBS sites for applications such as realtime ground motion predictions as front detections.
Abbreviations
 DNL:

degree of nonlinearity
 DONET:

dense oceanfloor network system for earthquakes and tsunamis
 JMA:

Japan Meteorological Agency
 KiKnet:

Kiban Kyoshin network
 KNET:

Kyoshin network
 OBS:

ocean bottom seismographs
 PGA:

peak ground acceleration
 SH/V:

Swave horizontal to vertical
 Snet:

seafloor observation network for earthquake and tsunami along the Japan Trench
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Authors’ contributions
YPD analyzed the data, interpreted the results, and drafted the manuscript. SA took part in the interpretation of the results and design of the study. TK, WS, and TK took part in the design of the study. All authors read and approved the final manuscript.
Acknowledgements
We would like to thank the Japan Meteorological Agency for providing us with hypocenter information of the earthquakes used in this study. We are grateful to two anonymous reviewers for their constructive and helpful comments that improved the quality of the manuscript. We also are grateful to Yasuo Ogawa, EditorinChief, Masato Furuya, Editor, and KuoLiang Wen, Lead Guest Editor, at Earth, Planet and Space for facilitating the review of this manuscript. We also would like to thank Wessel and Smith (1998) for providing us with Generic Mapping Tools, which were used to make some figures in this manuscript.
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The authors declare that they have no competing interests.
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Additional files
40623_2017_615_MOESM2_ESM.pdf
Additional file 2. Example plot of SH/V spectral ratios for different groups of PGAs at the KNG201 site.
40623_2017_615_MOESM3_ESM.pdf
Additional file 3. Comparison between weakmotion and strongmotion SH/V spectral ratios at the KNG202, KNG204, KNG205, and KNG206 sites.
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Dhakal, Y.P., Aoi, S., Kunugi, T. et al. Assessment of nonlinear site response at ocean bottom seismograph sites based on Swave horizontaltovertical spectral ratios: a study at the Sagami Bay area KNET sites in Japan. Earth Planets Space 69, 29 (2017). https://doi.org/10.1186/s4062301706155
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DOI: https://doi.org/10.1186/s4062301706155
Keywords
 Ocean bottom seismograph
 Nonlinear site response
 Horizontaltovertical spectral ratio
 Sagami Bay