- Express Letter
- Open Access
Geodetically estimated location and geometry of the fault plane involved in the 2018 Hokkaido Eastern Iburi earthquake
© The Author(s) 2019
- Received: 6 March 2019
- Accepted: 22 May 2019
- Published: 31 May 2019
- 2018 Hokkaido Eastern Iburi earthquake
- Crustal deformation
- Fault model
The 2018 earthquake occurred on the western edge of the thrust fault system. It should be noted that an active fault zone, called the Ishikari-Teichi-Toen fault zone (ITTFZ), is located close to the source region (Headquarters for Earthquake Research Promotion, HERP, 2010) (Fig. 1). According to HERP (2010), the ITTFZ consists of two parts: the main part (hereafter called ITTFZ-M), which is indicated by red solid lines in Fig. 1, and the southern part (hereafter called ITTFZ-S), indicated by red dotted lines. The long-term earthquake probability for the ITTFZ-S within the next 30 years is estimated as 0.2%, which is relatively high compared to other active faults in Japan. The source region of the 2018 earthquake is located near the ITTFZ-S and the southern tip of the ITTFZ-M, thus it is a controversial point if the 2018 seismic event occurred as a part of the fault system of the ITTFZ or not. The detailed source properties of this seismic event are fundamental information needed to further discuss the relationship of this event to the regional tectonics.
An L-band synthetic aperture radar (SAR) satellite, known as the Advanced Land Observing Satellite 2 (ALOS-2), makes observations for the purpose of detecting crustal deformation using SAR interferometry (InSAR). InSAR data have often revealed the source properties of not only large earthquakes but also moderate-sized inland earthquakes with magnitudes of ~ 6 due to the high spatial resolution of the data (e.g., Kobayashi 2017; Kobayashi et al. 2017). InSAR is capable of detailed mapping of crustal deformation as a rapid response to a seismic event, which will provide information about the spatial features of the fault rupture. The primary purpose of this study is to rapidly report the rupture location and style of the Eastern Iburi earthquake by retrieving crustal deformation data, and to discuss its relationship to the region’s seismo-tectonic setting.
SAR data and analysis method
We used ALOS-2 data from three orbits (Additional file 1: Table S1) for calculation. These observations were all conducted in stripmap mode with a spatial resolution of 3 m. To obtain the ground deformation, we applied an InSAR method to the data. Long spatial wavelength signals, which are presumably due to ionosphere-related noise, are included in the InSAR results. To reduce ionospheric noise, we applied a range split-spectrum method (Rosen et al. 2010; Gomba et al. 2016). We also reduced atmosphere-related noise using a numerical weather model; JMA mesoscale model (Kobayashi et al. 2014; Kobayashi 2016). The ALOS-2 data were processed using the GSISAR software (Fujiwara and Tobita 1999; Fujiwara et al. 1999; Tobita et al. 1999; Tobita 2003). After data processing, we obtained three InSAR images (Additional file 2: Fig. S1a, S1d, and S1 g).
We obtained multiple independent displacement components of InSAR data, in which the microwaves are emitted from two opposing directions: from the eastern sky and the western sky. This allowed us to convert the derived displacements into two components, which are quasi-up–down (QUD) and quasi-east–west (QEW) components (Fujiwara et al. 2000). We used the two InSAR datasets depicted in Additional file 2: Fig. S1a and S1 g for this analysis.
In addition to SAR-derived ground deformation data, we utilized data from the GNSS Earth Observation Network (GEONET) which has been deployed nationwide and is operated by the Geospatial Information Authority of Japan to obtain coseismic displacement vectors (Fig. 1) for the 2018 event. Note that the mounting pillars at two sites are tilted slightly as a result of the earthquake: sites 950132 (Atsuma) and 950141 (Monbetsu). The pillars are tilted with azimuth directions of 110° for 950132, and 200° for 950141. The azimuth is measured clockwise from north. The horizontal displacements caused by these inclinations were measured as 1.9 cm and 1.4 cm for 950132 and 950141, respectively. Thus, we corrected the coseismic displacements obtained from GNSS by subtracting the apparent displacements due to pillar inclinations at these two sites.
Some displacement discontinuities, indicated by arrows (Fig. 2b), can be observed in the QEW map, across which eastward and westward motions are located on the western and the eastern sides, respectively. In contrast, few clear discontinuities are found in QUD map. The details regarding these discontinuities are outside the scope of this study and will be discussed in Fujiwara et al. (2019).
Coseismic displacements were also recorded by GEONET deployed in and around the source region (Fig. 1), which agree with the spatial pattern we derived from the InSAR data. Note that it appears as though the displacement at site 950141 is opposite of the InSAR result: downward ground motion (3.4 cm) is visible within the uplift area. The amount is much larger than the downward movement resulting from the pillar inclination: ~ 0.02 mm. However, by zooming in on the QUD map (Additional file 3: Fig. S2), we can identify significant local subsidence in and around the GNSS site. It is possible that this site was affected by the local ground subsidence.
Fault model with a uniform slip
We constructed a fault model by assuming the presence of a rectangular fault with a uniform slip in an elastic half space (Okada 1985). We estimated the model parameters using a simulated annealing method, following the general procedure of Kobayashi et al. (2012). Taking into consideration the distribution of aftershocks (Fig. 1), the strike was searched from − 30° to +30°. For other parameters, we assigned search ranges of 141.8°–142.2° in longitude, 42.5°–42.8° in latitude, 0–50 km in depth, 0–20 km in length, 0–20 km in width, and 0–3 m in slip amount. Also, considering that the aftershock distribution is tilting downward to the east (HERP 2018), we have assumed an east-dipping in this model. Neither the dip angle nor the rake angle was constrained.
For the fault modeling, we used the three pairs of InSAR data (Additional file 2: Fig. S1). We calculated the variance of the displacement field outside the source region, where no deformation appeared, and regarded it as the variance for the study area. Consequently, for the weight, we assigned standard deviations of 2.1, 1.1, and 0.9 cm in line-of-site (LOS) component for InSAR paths 18, 116, and 122, respectively.
We also utilized GNSS data for our model, using standard deviations of the time series data for the weight: on average 0.2, 0.3, and 0.9 cm for E-W, N-S, and U-D components, respectively. Furthermore, we reduced the weight of sites 950132 and 950141 to suppress the local effect caused by the tilted pillars.
Fault parameters for a fault model with a uniform slip. The location of the fault is indicated in the top-left corner
There is an obvious inconsistency for site 950141 between the observation and the model prediction: the vertical movement is not consistent between the data and the model. As mentioned previously, this area could have been subjected to not only fault-related crustal deformation but also local deformation. This local effect likely culminated in the bad data fitting.
The beach ball plot estimated from the fault model is shown in Fig. 2c, which is consistent with the seismically determined focal mechanism (Fig. 1), while seeing the details, non-double couple component is significantly included in the CMT solution. It may suggest that fault ruptures with a complex geometry system is involved with this seismic event rather than a single fault plane (Himematsu and Furuya 2016; Kobayashi 2017) although there is no clear signal suggesting the complexity in the geodetic data.
The source fault’s association with the ITTFZ
The estimated fault plane has a high dip angle (74°). If the fault plane extends to the ground surface with the same dip angle, the fault top would be located to the east of the known fault traces of the ITTFZ, suggesting that the fault plane for this event does not directly connect to the ITTFZ. One possibility is that the fault plane for the 2018 event is physically separate from the ITTFZ and the ITTFZ was not involved at all in the 2018 event. On the other hand, according to seismic surveys, there are some reflection planes with low angles at shallow depths in the ITTFZ (HERP 2010). If we assume both the fault that caused the 2018 event and the known ITTFZ are part of one fault system, the dip angle should turn out to be lower at shallow depth for the fault that caused the 2018 event (Fig. 3c). In this study, we claim only that this speculation is not inconsistent with the limited available data/knowledge, and it seems geophysically and geologically reasonable for the region. The fault slip terminated at approximately ~ 15 km in depth, and thus it is difficult to exploit further information regarding fault structure from geodetic data. To deepen the discussion of this topic, more detailed information on regional crustal structures is needed in the future.
Comparison to velocity structure
Seismic surveys have revealed that earthquakes often occur at anomalous area of seismic velocity (e.g., Kato 2013). Also, in the Hidaka collision zone, large historical intraplate earthquakes occurred in and around anomalous velocity areas (Kita et al. 2012). Thus, it is possible that there is some relationship between the 2018 event and crustal structure. We examined the velocity structure in and around the source region. Figure 3a–c shows the spatial distribution of P-wave (Vp) speed (Matsubara and Obara 2011; Matsubara et al. 2017). These profiles cut through the central part of the estimated fault model. A black-colored frame projected on each profile represents the fault plane. First, we find that the low and high Vp areas are distributed on the eastern and western sides of the source region, respectively (Fig. 3a). In the vertical profile in the longitudinal direction (Fig. 3c), the low Vp area thickens on the eastern side of the fault, and the fault slip is positioned at the western edge of the low Vp. It is noted that the Vp-stratified structure is tilted downward to the east at and around the fault, and it is consistent with the dip angle of the estimated fault plane. Also, when compared to the Vp/Vs ratio (Additional file 7: Fig. S6), we identify that low Vp/Vs is distributed on the eastern side of the slip area, which may suggest involvement of water/fluid (Nakajima et al. 2001). The anomalous structure may suggest that the 2018 seismic event occurred at seismic velocity boundary.
Hypocenter estimate, in general, could be strongly by local structures (e.g., Melgar et al. 2018). The seismic velocity contrast indicates a shear modulus change across the fault. The lower shear modulus on the east side may push the hypocenters further to the west, which culminates in the above-mentioned spatial inconsistency between the geodetically and the seismically determined positions.
Effect of stress change on the ITTFZ
The crust in the proximity of the ruptured fault should have been subjected to a strong stress change during the 2018 event, which presumably culminated in the promotion of other earthquakes. To test this idea quantitatively, we evaluated Coulomb Failure Function change (ΔCFF) values (King et al. 1994). We assumed a receiver fault with a reverse motion on a fault plane dipping to the east with the dip angle of 10° (HERP 2010). We placed a receiver fault along the ITTFZ with a strike of 340°, which is measured clockwise from north, at a fault top depth of 5 km, indicated by the white frame in Fig. 3a. Figure 3d shows the ΔCFF estimates. Warm and cool colors represent positive and negative signs, indicating facilitated or suppressed fault slip, respectively. We set an effective coefficient of friction μ of 0.4. In most regions of the ITTFZ-S, the ΔCFF values tend to be positive. On the other hand, at the southern and northern tips of the ITTFZ-S, the ΔCFF values are negative. We attempted to evaluate the stability of our stress change pattern for an effective coefficient of friction from 0.2 to 0.8, and confirmed that in all cases the spatial patterns are substantially the same (Additional file 8: Fig. S7b, e, h). In addition, we evaluated the stability for a fault top depth from 0 to 10 km. In all cases, reverse slip tends to be promoted in the central part of the ITTFZ-S, while in the northern and southern tips of the ITTFZ-S, the promotion/suppression of slip is sensitive to fault depth. At this stage, we can say at least that the slip could be promoted on the central part of the ITTFZ. Of course, care must be taken with these estimates because the source and the receiver faults are close together, and thus our estimates can be sensitive to position and the given slip mechanism. To evaluate it more thoroughly, more detailed locations and fault geometries of the ITTFZ will be needed.
Uplift of up to ~ 7 cm is predominantly distributed in the source region, and eastward movement of up to ~ 4 cm is widely observed on the eastern side of the source region.
The fault model shows that the fault plane extends in a north–south direction and is dipping to the east with a dip angle of 74°. The fault plane has a relatively high dip angle, and the shallow extension of the estimated fault plane does not directly connect to any known surface traces of the ITTFZ.
The fault model shows a reverse fault motion with a Mw 6.6. The fault top is positioned at around 15 km in depth, suggesting that the slip significantly occurs deeper than the typical seismogenic zone for the Japanese island (~ 15 km).
The estimated fault is located in a region of anomalous seismic velocity, possibly suggesting that the 2018 earthquake occurred at seismic velocity boundary.
A ΔCFF estimate suggests that the static stress change due to the Eastern Iburi earthquake can promote reverse slip in the central region of the ITTFZ-S. For the northern and southern tip of the ITTFZ-S, slip can be suppressed in some cases due to sensitivity to fault depth.
ALOS-2 data were provided by the Earthquake Working Group under a cooperative research contract with Japan Aerospace Exploration Agency (JAXA). The ownership of ALOS-2 data belongs to JAXA. We used the software “Hi-net 3D Tomography Viewer (Ver. 3.0)” to plot the velocity structure. Hypocenter data processed by the Japan Meteorological Agency (JMA) were used. Generic Mapping Tools (GMT) (Wessel and Smith 1998) were used to construct the figures.
TK analyzed the InSAR data, constructed the fault models, and drafted the manuscript. KH produced the InSAR data. HY discussed the results and managed the study. All authors read and approved the final manuscript.
The authors declare that they have no competing interests.
Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
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