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Source rupture process of the 2018 Hokkaido Eastern Iburi earthquake deduced from strong-motion data considering seismic wave propagation in three-dimensional velocity structure
Earth, Planets and Space volume 71, Article number: 101 (2019)
The source rupture process of the 2018 Hokkaido Eastern Iburi earthquake (MJMA 6.7) was analyzed by a kinematic waveform inversion method using strong-motion data in 0.04–0.5 Hz. This earthquake occurred close to the Hidaka Collision Zone and the Ishikari depression, where the crustal structure is rather complex. Thus, we used a three-dimensional velocity structure model to compute the theoretical Green’s functions by the finite difference method. A source fault model with strike-angle variation was set based on the spatial distribution of the early aftershocks. The strong-motion stations used for the source inversion were selected based on the result of forward ground motion simulation of a moderate aftershock. The slip in the first 5 s was relatively small, but an area of significant slip with peak slip of 1.7 m was found in the depth range from 22 to 32 km. The rupture propagated upward mainly in the southwest direction. Based on the regional crustal structure and the configuration of the Moho discontinuity, the large-slip area was thought to be located in the lower crust, and its rupture did not reach the upper part of the continental crust. Most of the early aftershocks occurred around the large-slip area. The later aftershocks at the depth shallower than 20 km occurred outside the causative source fault of the mainshock. Three-dimensional ground motion simulation demonstrated that the heterogeneous source process and the three-dimensional basin and crustal velocity structure brought a large velocity pulse to an area to the southwest of the source fault, where the largest PGV was observed during the mainshock. The spatial distribution of the simulated PGV resembled the observed PGV distribution except some sites located inside the Ishikari depression where thick Quaternary soft low-velocity sediments exist at the top of the basin.
Hokkaido Island was rocked by an MJMA 6.7 earthquake, called the 2018 Hokkaido Eastern Iburi earthquake. It occurred to the west of the Hidaka Collision Zone, Central Hokkaido, Japan, at a depth of 37 km, at 03:08 JST on September 6, 2018 (18:08 UTC on September 5, 2018) (Fig. 1). This earthquake drew significant attentions to a number of landslides in the epicentral region (Yamagishi and Yamazaki 2018; Yamaguchi et al. 2019), liquefaction in residential areas in Sapporo and other cities (Hirose et al. 2018; Karimzadeh and Matsuoka 2018; Kuwahara et al. 2018), and blackout in the whole Hokkaido Island (Ozaki et al. 2019). An overview of casualties, damages and government responses was reported by Takahashi and Kimura (2019).
The hypocenter of the 2018 Hokkaido Eastern Iburi earthquake is located by the Japan Meteorological Agency (JMA) beneath the western part of the Hidaka Collision Zone, which is an arc–arc collision system in Hokkaido Island. The Kuril forearc sliver moved southwestward since the Late Miocene and collided with the Northeast Japan Arc due to the oblique subduction of the Pacific plate (Kimura 1986). This tectonic setting makes the high-velocity Hidaka body thrust steeply over the low-velocity crust of the Northeast Japan Arc at the western edge of the Kuril forearc (Arita et al. 1998; Iwasaki et al. 2004; Kita et al. 2012; Moriya et al. 1998). Mature continental-type crust of the Kuril Arc has been exposed in the Hidaka Mountains as a result of collision (Kimura 1996). The collision of the Kuril forearc sliver is also developing the foreland fold-and-thrust belt with very thick sedimentary basins to the west of the Hidaka Mountains. The westernmost part of this belt is called the Ishikari depression (Ishikari Lowland) (Iwasaki et al. 2004; Kimura 1996). Accordingly, the crustal structure in this region is rather complex due to the above-mentioned situation. Recently, Kita et al. (2012) imaged P- and S-wave velocity structure by a travel-time tomography technique and concluded that the arc–arc collision of this region produced M7-class earthquakes at anomalously deep depths at sharp material boundaries between uppermost mantle and crustal materials (MJMA 6.7 Hidaka earthquake at 55 km on January 21, 1970 and MJMA 7.1 Urakawa-oki earthquake at 40 km on March 21, 1982). The 2018 Hokkaido Eastern Iburi earthquake could be thought to be one of such anomalously deep earthquakes in the Hidaka Collision Zone.
The strong ground motions during this event were observed by nation-wide and regional strong-motion networks. We have collected strong-motion data from K-NET, KiK-net, and F-net of the National Research Institute for Earth Science and Disaster Resilience (NIED) (Aoi et al. 2011; National Research Institute for Earth Science and Disaster Resilience 2019a, b; Okada et al. 2004), and seismic intensity observation networks operated by JMA, Hokkaido Government, and City of Sapporo (Nishimae 2004). The observed PGA exceeded 1500 cm/s2 at KiK-net IBUH01 and K-NET HKD127 both located in Oiwake of Abira town, Yufutsu District, Iburi Subprefecture. The site is in Yuni-Abira Lowlands, which is a narrow valley, the eastern part of the Ishikari depression. The observed PGV exceeded 100 cm/s at several strong-motion stations in Mukawa, Atsuma, and Abira towns. The largest one among the collected data was the record at station HKD126 in Mukawa, which is a coastal town known for Shishamo fish, in the east of the Yufutsu basin. Seismic intensity of 7 in JMA scale was recorded during this event at one JMA seismic intensity station (station code 41407 in Atsuma town). Figure 2 shows velocity waveforms observed at strong-motion stations in the vicinity of the epicenter. These velocity waveforms were processed by integrating the original acceleration waveform data observed at those stations, and bandpass-filtered in the frequency range from 0.05 to 20 Hz. Manually picked onset times of P- and S-waves are indicated by blue and red triangles in this figure. The observed records clearly show difference in arrival time between the initial S-wave onset and the largest amplitude (Fig. 2 and Additional file 1: Fig. S1). The fact indicates the possibility that the initial part of the source fault rupture was weak and significant slips generating strong ground motions occurred shortly afterward. The arrival time of the largest amplitude is the earliest at station 47004, which implies that seismic source generating this pulse is relatively close to this station.
The spatial PGA and PGV distributions show larger amplitude to the west of the source region, particularly in the Yufutsu and Ishikari basins, both are part of the Ishikari depression. The large amplification of long-period ground motions in the Yufutsu sedimentary basin was also observed during the 2003 Tokachi-oki earthquake (MW 8.3) causing severe damages to large oil storage tanks in Tomakomai by liquid sloshing (Aoi et al. 2008; Hatayama et al. 2007; Koketsu et al. 2005; Maeda and Sasatani 2004). The Ishikari depression including the Ishikari and Yufutsu sedimentary basins has exceptionally thick Quaternary to Paleogene sediments, whose depth to the Early Cretaceous bedrock is around 8 km (Aoi et al. 2008; Yokokura et al. 2014). Thus, the effects of the three-dimensional sedimentary and crustal structure on the seismic waves need to be considered while studying the source rupture process using regional strong-motion data.
In this paper, the source rupture process of the 2018 Hokkaido Eastern Iburi earthquake is deduced from strong-motion data by a kinematic waveform inversion method. Because of the above-mentioned reasons, we also considered a three-dimensional velocity structure model in the source inversion analysis. The obtained source rupture process will be discussed with respect to the crustal structure and the spatiotemporal aftershock distribution. Then, a three-dimensional ground motion simulation demonstrates spatial distribution of ground motions focusing attention on the effects of the heterogeneous source rupture process and the three-dimensional underground velocity structure.
Finite source inversion method and source fault model setting
The kinematic source rupture process of this earthquake was analyzed by the multiple time-window linear waveform inversion method developed by Hartzell and Heaton (1983) and Olson and Apsel (1982). The observational equation of this problem is based on the representation theorem (Maruyama 1963; Burridge and Knopoff 1964). The same technique has been widely applied to strong-motion data for many past large earthquakes (e.g., Asano and Iwata 2016; Ma et al. 2001; Sekiguchi et al. 2000; Suzuki et al. 2011; Wald and Heaton 1994; Yoshida et al. 1996). Our source inversion code has been tested in the Source Inversion Validation project (Gallovič and Ampuero 2015; Mai et al. 2016).
A source fault model was assumed by referring to the spatial distribution of the early aftershocks in the JMA unified hypocenter catalog, which is presented in Fig. 3. The aftershocks occurring within 2 h from the mainshock’s origin time were plotted in this figure. Most of the aftershocks in this time-period occurred at the depth deeper than 30 km. The early aftershock distribution shows clearly a steep fault plane dipping eastward. The strike angle of the source fault changes along the strike direction like a byobu (Japanese folding screen with two or more panels). Thus, we assumed a source model which consists of three fault planes by changing strike angle. The dip angle is assumed to be 70° referring to the aftershock distribution and the centroid–moment tensor solution of Global CMT Project (Ekström et al. 2012). The assumed source fault model is also plotted in Fig. 3.
The fault plane model was divided into small equal-area subfaults (3 km × 3 km). The temporal moment-release history at the center of each subfault was represented by several time-windows. The unknown model parameters in this source inversion analysis were the amplitude of the basis functions corresponding to each time-window at each subfault. The number of the time-windows at each subfault was set at 4 after preliminary analysis. The rupture front of the first time-window propagated radially at a constant velocity from the rupture starting point fixed at the hypocenter, and we assumed that the rupture propagates continuously beyond the segment boundary. Since each time-window at each subfault has two orthogonal rake angles to represent variable rake angle, the total number of the unknown model parameters was 80 × 4 × 2 = 640. The rake angle variation was limited within a certain range, as described in Table 1. The problem could be solved using the linear least-squares method with a nonnegative constraint (Lawson and Hanson 1974). A spatiotemporal smoothing constraint was included following Sekiguchi et al. (2000) to stabilize the solution. A relative weight of the smoothing constraint equation against the observational equation and the rupture propagation velocity triggering the first time-window were determined so as to minimize the Akaike’s Bayesian information criterion (ABIC) (Akaike 1980).
Strong-motion data and Green’s function based on a three-dimensional velocity structure model
As briefly described in the introduction of this paper, the crustal and sedimentary basin structure is complex, and it would significantly affect the seismic wave propagation and amplification in this area. Thus, it is desirable to prepare theoretical Green’s functions describing the seismic wave propagation in a three-dimensional crustal and basin structure. There are pioneering works for kinematic source inversion studies of strong-motion records using three-dimensional velocity structure model (e.g., Graves and Wald 2001; Liu and Archuleta 2004). Graves and Wald (2001) concluded that the use of well-calibrated Green’s functions calculated for a three-dimensional velocity structure had the potential for increased resolution of the rupture process. Thanks to development of detailed three-dimensional velocity structure models and improvement of computing facilities, nowadays the application of three-dimensional velocity structure model is being practical (e.g., Gallovič et al. 2015; Guo et al. 2013; Hsieh et al. 2016; Kubo et al. 2016; Lee et al. 2016; Somala et al. 2018; Yun et al. 2016).
In this study, the theoretical Green’s functions were computed by the three-dimensional finite difference method (FDM) using a three-dimensional velocity structure model, the Japan Integrated Velocity Structure Model Version 1 (JIVSM; Koketsu et al. 2012). This velocity structure model is represented by a stack of isotropic homogeneous layers from near-surface sedimentary layers to subducting oceanic plates, and each of the layer boundaries was modeled by integrating many kinds of geophysical exploration data and seismic wave modeling (Koketsu et al. 2012). Figure 4 shows the bedrock (VS = 2.9 km/s) depth distribution and a west–east cross-section of JIVSM. The model reflects lateral variation produced by the Hidaka Collision Zone and the foreland fold-and-thrust belt. Area to the west and south of the epicenter has relatively thick Quaternary to Paleogene sediments. The lowest S-wave velocity of the above-mentioned model is 0.6 km/s in the area shown in the map. That is, Holocene and Upper Pleistocene layers which may have S-wave velocity lower than 0.6 km/s are not included in the present velocity model for this area.
A staggered-grid FDM code, which has been coded and used in Asano et al. (2016), was used to compute the Green’s functions. This code solves the elastodynamic wave equation in a velocity–stress formulation with fourth-order accuracy in space and second-order accuracy in time. The FDM model space, occupying an area of 190 km (E–W) × 200 km (N–S) in southern and central Hokkaido corresponding to the geographical area shown in Fig. 4, extends to a depth of 80 km below the ground surface. The model was discretized using a uniform grid of 0.1 km along the horizontal and vertical axes. The total number of the grid points was 1901 × 2001 × 802 = 3,050,728,602. The boundary condition between the isotropic homogeneous layers was introduced by adopting the technique of Moczo et al. (2002). A zero-stress formulation was introduced for the free surface boundary condition at the top of the model space (e.g., Levander 1988; Graves 1996). A multi-axial perfectly matched layer (PML) was applied to the model boundaries, except for the free surface, to avoid non-physical reflections (Meza-Fajardo and Papageorgiou 2008; Zeng et al. 2011). The grid thickness of the PML domain was set at 10 grids. Anelastic attenuation in the medium was included in the form of a linear frequency-dependent Q operator Q(f) = Q0(f/f0) following the method proposed by Graves (1996). The reference frequency f0 is set at 0.5 Hz. The three-dimensional wave propagation was simulated for 80 s after the origin time at increments of 0.005 s, which made the total number of time steps in a simulation be 16,000.
To choose strong-motion stations for the source inversion analysis, we first simulate ground motions for an MW 4.1 aftershock, which occurred at 9:48 on September 14, 2018 (JST). The epicenter location of this aftershock was given referring to the JMA unified hypocenter catalog. A point source moment tensor was assumed for as the source term, and we used the moment tensor solution of F-net, NIED. The source parameters of this aftershock are summarized in Table 2. At the KiK-net stations (station code of IBUHxx, HDKHxx, IKRHxx, SRCHxx), observed records from downhole sensors, were used for this analysis to avoid effects of very soft sediments. The broadband sensors of F-net were installed in an observational tunnel at each station (HID and HSS), and the strong-motion sensors of the K-NET stations (HKDxxx) were installed on the ground surface. The original acceleration records were numerically integrated in the time domain to obtain the velocity records except the F-net stations being equipped with a velocity-type strong-motion seismograph. Some near-source strong-motion stations to the west of the epicenter such as HKD126, HKD128, 47004, and 51200 were excluded in the source inversion analysis because those ground motion records were strongly affected by the nonlinear effects of the near-surface soil material during extremely strong shaking (e.g., Dhakal et al. 2019; Ikeda and Takagi 2019; Takai et al. 2019).
After inspecting waveform fitting at strong-motion stations in central and southern Hokkaido, we finally chose 16 strong-motion stations of K-NET, KiK-net and F-net shown by the solid triangles in Fig. 1a. The comparison between the observed and simulated velocity waveforms at those strong-motion stations is presented in Additional file 2: Fig. S2. The simulated waveforms using the three-dimensional velocity structure model for the selected stations (Additional file 2: Fig. S2) are better than the simulated waveforms using the one-dimensional velocity structure model (Additional file 3: Fig. S3) particularly in terms of elongation of the ground motion duration by the three-dimensional effects. Those 1D synthetics were calculated by the discrete wavenumber method (Bouchon 1981) with the reflection and transmission matrix (Kennett and Kerry 1979), and the one-dimensional velocity structure model for each station is constructed by extracting the one-dimensional profiles beneath the site from JIVSM. Thus, the near-surface response was common between 1D and 3D modeling. If we use an identical one-dimensional velocity model for all the stations, waveform fitting would become much worse than Additional file 3: Fig. S3.
Then, the Green’s functions for the source inversion of the mainshock were computed by FDM. Since each subfault must have two orthogonal slip components (90° and 0°), the total number of the required computing runs was 160. Both observed velocity waveforms and synthetic Green’s functions were bandpass-filtered from 0.04 to 0.5 Hz, and then resampled at 5 Hz. Forty-second length of the velocity waveform starting from 1 s before the initial S-wave arrival was used for the source inversion analysis. The initial S-wave arrival of both observed and synthetic waveforms was picked up carefully by visual inspection to make the timing of the S-wave onset same among the waveforms and to compensate the residual between the observed and theoretical travel times. Examples of the manual picking for the observed waveforms are demonstrated in Additional file 1: Fig. S1.
Figure 5 shows the estimated final slip distribution. This source model has a seismic moment of 1.99 × 1019 Nm (MW 6.8). The synthetic waveforms explain characteristics of the observed waveforms fairly well (Fig. 6). The snapshot at every 1 s was plotted as map view in Fig. 7. The slip in the first 5 s was small; then, the rupture propagated upward in the southwest direction. The rupture also spread to the north afterward. The entire rupture finished within 15 s. The best estimate for the propagation velocity triggering the rupture front of the first time-window was 1.8 km/s. The peak slip reaching 1.7 m was found at a depth of about 26 km, southwest of the epicenter. The average slip over the source fault was 0.59 m. The slip-weighted average rake angle over the entire fault was 103°, which was similar to the published moment tensor solutions by the Global CMT project (strike 349°, dip 68°, rake 102°) and NIED F-net (strike 349°, dip 65°, rake 107°). There were relatively large slips at the south-bottom edge of the assumed source fault. Generally, it is not easy to judge whether such a large slip near the edge of the assumed source fault is true slip or artifact. But, the contribution of that slip to the waveforms is not significant.
Significant slip larger than 1 m was estimated in the depth range from 22 to 32 km. Hereafter, we call it large-slip area. The Moho depth around the epicenter in JIVSM is approximately 32 km. Matsubara et al. (2017) also published a digital map of the Moho discontinuity beneath the Japanese Islands derived from three-dimensional seismic tomography. In their model, the depth of the Moho discontinuity in the source region of the 2018 Hokkaido Eastern Iburi earthquake is also 32–34 km, and it slants gradually down to the south. Besides, the hypocenter is close to the profile A in Fig. 6 of Kita et al. (2012), and their model also imaged the Moho discontinuity at depth around 32–34 km. The fault rupture stopped at a depth of about 20 km, which was deeper than the upper and lower crust boundary. Therefore, the rupture of the 2018 Hokkaido Eastern Iburi earthquake initiated at nearly top of the upper mantle, and the small slips in the first 5 s correspond to the early stage of the rupture occurring below the Moho discontinuity. Then, the large slip occurred in the depth range from 32 to 22 km within the lower crust. These temporal rupture characteristics were quite consistent with the characteristics of the observed waveforms in the near-source region as mentioned in the introduction. In this regard, this earthquake is different from most Japanese crustal earthquakes, which usually occur in the upper crust.
The 1982 Urakawa-oki earthquake (MJMA 7.1, MW 6.9) occurred at 42.07°N, 142.60°E at a depth of 40 km on the deep extension of one of thrust faults belonging to the Ishikari Lowland Eastern Edge Fault System (Kita et al. 2012). The source fault of the 1982 Urakawa-oki earthquake was a thrust fault dipping to northeast (Suetsugu and Nakanishi 1988). The geometry and depth range of the source fault of the 2018 Hokkaido Eastern Iburi earthquake were similar to that of the 1982 Urakawa-oki earthquake. Both of the earthquakes are thrust events in the lower crust under the common tectonic condition controlled by the regional stress filed of the Hidaka Collision Zone.
Slip distribution of the mainshock and temporal aftershock distribution
The temporal aftershock distribution was compared with the final slip distribution (Fig. 8). The aftershock locations were taken from the JMA unified hypocenter catalog. Eight periods are shown in this figure. The location of the largest aftershock (MJMA 5.5), which occurred 12 min after the mainshock, was nearly southern edge of the source fault of the mainshock. It suggests a possibility that this largest aftershock was induced by the stress accumulation due to the rupture of the large-slip area during the mainshock. Most of the aftershocks occurring in the first 6 h were located surrounding the large-slip area, particularly in the deeper part of the mainshock’s source fault. Then, the aftershock activity in the depth shallower than 20 km becomes active. This temporal aftershock distribution also supports that the rupture of the mainshock did not reach the upper part of the crust, which is shallower than 20 km.
We have referred to the JMA unified hypocenter catalog, which is a homogeneous earthquake catalog covering the whole territory of Japan. A single one-dimensional velocity model was used for the inland earthquakes in the JMA catalog. Thus, the theoretical travel time calculated from the JMA velocity model may be different from the theoretical travel time calculated for each station from JIVSM. Generally, those theoretical travel times may not perfectly correspond to the observed travel time because of the local site effects and the Earth’s heterogeneities as seen in Additional file 2: Fig. S2. The initial S-wave arrival of both observed and synthetic waveforms were picked up carefully by visual inspection to compensate the residual between the observed and theoretical travel times in our source inversion analysis. Therefore, the difference in the assumed velocity structure model will not apparently affect the slip distribution because the spatiotemporal slip was solved relative to the hypocenter location and the origin time. Nevertheless, the application of the local velocity structure model makes us improve the reproductivity of waveforms itself and see more precise image of the source process (e.g. Asano and Iwata 2011).
Spatial distribution of ground motions during the mainshock
A forward ground motion simulation using FDM for the mainshock was carried out to demonstrate effects of the heterogeneous source rupture process and the three-dimensional velocity structure on the strong ground motions in central and southern Hokkaido. The geographical area for the FDM simulation (190 km × 200 km) is same as the computations of Green’s functions described before (Fig. 4). The kinematic source model obtained in this study was used for this FDM simulation. The output ground motions were obtained at the free surface (top of VS = 600 m/s layer in this model).
Figure 9 presents snapshots of the ground velocities in the EW component. The same figures for the NS and UD components are presented in Additional file 4: Fig. S4 and Additional file 5: Fig. S5, respectively. The geographical area of those maps corresponds to the FDM model space, which is represented by the broken rectangle in Fig. 4. At about 18 s after the origin time, a large amplitude velocity pulse (~ 20 cm/s), which is indicated by the black arrow in Fig. 9, hits the area to the southwest of the source fault, where large PGV was observed in Mukawa and Atsuma towns. This velocity pulse dominated in the EW component (Fig. 10). It was originated from the large-slip area, and it was amplified by the deep sedimentary layers in this area. But, the actual observed ground velocities at Mukawa (HKD126) and Atsuma (47004) (Fig. 2) were much larger than the simulated ground motions. It might be because that the present velocity structure model in this FDM simulation does not include near-surface Quaternary soft sedimentary layers, whose S-wave velocity is much lower than 0.6 km/s, as low as 0.1 km/s expected from the K-NET PS-logging information at HKD126 (National Research Institute for Earth Science and Disaster Resilience 2019a).
Since the ground motions were simulated at the top of engineering bedrock (VS = 0.6 km/s), the simulated ground motions could be interpreted as input motions at the bottom of shallow low-velocity layers. Existence of significant amplification by the shallow low-velocity layers is also evidenced by the amplitude difference in the observed ground motions at uphole and downhole sensors of IBUH01 plotted in Fig. 2.
Duration of ground motions was long in the Ishikari and Yuftusu basins, and the wave propagation inside those basins looks slow compared to the other directions (Fig. 9). Figure 11 compares the simulated PGV with the observed PGV in the frequency range lower than 0.5 Hz. The spatial pattern of the simulated PGV distribution resembles the observed PGV map except the sites located inside the Ishikari depression, where existence of thick Late Pleistocene to Holocene low-velocity sediments is expected (e.g., Sagayama et al. 2017; Sato and Komatsubara 2014). This result supports that the source model obtained in this study is adequate to model the ground motions in this frequency range.
As a future issue on the ground motion modeling in this area, investigation and modeling of the shallow low-velocity layers would be required for quantitatively evaluating the surface ground motions in the area with thick Quaternary sediments. Moreover, this FDM simulation was limited up to 0.5 Hz. Thus, it is also necessary to model the broadband ground motions by including the effects of near-surface low-velocity sediments for evaluating quantitatively the input ground motions to buildings and landslides in the disaster-affected area.
The source rupture process of the 2018 Hokkaido Eastern Iburi earthquake (MJMA 6.7) was estimated by the kinematic waveform inversion technique using strong-motion waveform data and three-dimensional velocity structure model. The theoretical Green’s functions were computed using a three-dimensional velocity structure model JIVSM by FDM to include the effects of wave propagation controlled by complex crustal structures such as the Hidaka Collision Zone and the foreland fold-and-thrust belt in the study region. The source fault was dipping to eastward with variation in strike angle. The result of the kinematic source inversion revealed that the initial rupture in the first 5 s was weak, and then rupture propagated up- and southwestward. The peak slip reaching 1.7 m was found at a depth of approximately 26 km to the southwest of the hypocenter. The total seismic moment was estimated to be 1.99 × 1019 Nm (MW 6.8). The large-slip area was restricted in the depth range from 22 to 32 km, which is in the lower crust. Thus, the rupture of the 2018 Hokkaido Eastern Iburi earthquake initiated at nearly top of the upper mantle, and propagated upward beyond the Moho discontinuity. The crustal structure might control such rupture characteristics of this earthquake as well as the 1982 Urakawa-oki earthquake (MW 6.9) occurring approximately 85 km southeast of the 2018 Hokkaido Eastern Iburi earthquake. More detailed works on the fault geometry and crustal structure may improve physical understanding of this earthquake and reproduction of the waveforms. The spatial extent of the causative source fault of the mainshock was also supported by the spatial and temporal distributions of aftershocks. The forward three-dimensional ground motion simulation demonstrated that the combination of heterogeneous source process and three-dimensional basin and crustal velocity structure brought a large velocity pulse to an area to the southwest of the source fault, where the largest PGV was recorded during the mainshock. The discrepancy between the simulated amplitude and the observed amplitude of the ground velocities would be due to thick Quaternary low-velocity sediments in the Ishikari depression, which was not included in the present velocity structure model. Further studies both on the broadband ground motion modeling and the effects of near-surface low-velocity sediments would help in evaluating the input ground motions to buildings and landslides.
Availability of data and materials
The acceleration waveform data of the strong-motion seismograph networks K-NET and KiK-net were provided by the National Research Institute for Earth Science and Disaster Resilience (NIED) via their website (http://www.kyoshin.bosai.go.jp). The broadband strong-motion velocity waveform data of F-net and Hokkaido University were downloaded from NIED Hi-net website (http://www.hinet.bosai.go.jp). The strong-motion data from the seismic intensity observation networks of the Japan Meteorological Agency (JMA), Hokkaido Government, and City of Sapporo were provided by them at the website of JMA (http://www.data.jma.go.jp/svd/eqev/data/kyoshin/jishin/1809060307_hokkaido-iburi-tobu/index.html). The JMA unified hypocenter catalog was published as the Seismological Bulletin of Japan by JMA in collaboration with the Ministry of Education, Culture, Sports, Science, and Technology (https://www.data.jma.go.jp/svd/eqev/data/bulletin/index_e.html). The Global Centroid Moment Tensor Project database is open to public at http://www.globalcmt.org. The post-processed SRTM 90 m Digital Elevation Database is hosted by the Consortium for Spatial Information of the Consultative Group for International Agricultural Research (CGIAR-CSI) at http://srtm.csi.cgiar.org/. The digital data of the kinematic finite source model estimated in this study will be deposited in SRCMOD Finite-Source Rupture Model Database (Mai and Thingbaijam 2014; http://equake-rc.info/SRCMOD/) after this paper is published.
Akaike’s Bayesian Information Criteria
finite difference method
Japan Integrated Velocity Structure Model
Japan Meteorological Agency
Japan Standard Time
National Research Institute for Earth Science and Disaster Resilience
peak ground acceleration
peak ground velocity
perfectly matched layer
coordinated universal time
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The Cray XC40 supercomputer of the Academic Center for Computing and Media Studies of Kyoto University was used for computing the theoretical Green’s functions. All figures were drawn using the Generic Mapping Tools v. 5.4.4 (Wessel et al. 2013). The comments from two anonymous reviewers were helpful for improving this paper.
This study was supported by the Grant-in-Aid for Special Purposes 18K19952 (PI: Prof. Hiroaki Takahashi at Hokkaido University) from MEXT (Ministry of Education, Culture, Sports, Science, and Technology) and the Earthquake and Volcano Hazards Observation and Research Program of MEXT, and the collaborative research program of the Disaster Prevention Research Institute, Kyoto University (30A-03).
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Additional file 2: Fig. S2. Comparison of the observed velocity waveforms (black traces) and the synthetic velocity waveforms using JIVSM (red traces) in 0.04–0.5 Hz for the MW 4.1 aftershock at 09:48 on September 14, 2018. The amplitudes were normalized by the maximum observed amplitude. The maximum observed amplitude of each component is shown above each trace in units of cm/s. NS north–south, EW east–west, UD up–down.
Additional file 3: Fig. S3. Comparison of the observed velocity waveforms (black traces) and the synthetic velocity waveforms using station-dependent 1D velocity models (red traces) in 0.04–0.5 Hz for the MW 4.1 aftershock at 09:48 on September 14, 2018. The amplitudes were normalized by the maximum observed amplitude. The maximum observed amplitude of each component is shown above each trace in units of cm/s. NS north–south, EW east–west, UD up–down.
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Asano, K., Iwata, T. Source rupture process of the 2018 Hokkaido Eastern Iburi earthquake deduced from strong-motion data considering seismic wave propagation in three-dimensional velocity structure. Earth Planets Space 71, 101 (2019) doi:10.1186/s40623-019-1080-0
- The 2018 Hokkaido Eastern Iburi earthquake
- Source rupture process
- Kinematic source inversion
- Strong-motion data
- Three-dimensional velocity structure
- Ground motion simulation