## Abstract

Our moment tensor inversion of the 2011 Tohoku-Oki earthquake, using regional broadband strong-motion waveforms, indicates that the earthquake can be approximated by a point source. The amplitude spectra of the observed displacement seismograms were fitted by the omega-square model, which resulted in the corner frequency of around 0.016 Hz. This implies a large slip over a circular fault having a radius of 70 km, with a rupture duration of about 40 s. The moment-rate function estimated from the inversion shows a large impulse of similar duration. We interpret this impulse to correspond to the rupture estimated from the corner frequency. From the seismic moment released during the impulse, we have estimated the average slip and stress drop over the fault to be 50 m and 40 MPa, respectively. This stress drop corresponds to an effective normal stress larger than 200 MPa, indicating that a strong localized asperity (mega asperity) was ruptured during the earthquake. Previous simulation studies suggested the importance of a large effective normal stress at a shallow plate interface, which was explained by a pore pressure distribution along the plate. We have explored the possibility of a subducted seamount to be the origin of the mega asperity.

## 1. Introduction

One of the serious questions raised by the Tohoku-Oki earthquake of 11 March, 2011, is why the mega earthquake occurred in the subduction zone along the Japan Trench, where the plates were believed to be weakly coupled (e.g., Kanamori, 1986). Various slip models for the Tohoku-Oki earthquake have been proposed from seismic, GPS, and tsunami, data analyses (e.g., Fujii *et al.*, 2011; Ide *et al.*, 2011; Lay *et al.*, 2011; Ozawa *et al.*, 2011; Simons *et al.*, 2011). However, these slip models display a large variability, which may reflect the non-uniqueness of an under-determined inverse problem of solving the slip distribution over a finite fault (e.g., Simons *et al.*, 2011). On the other hand, recent models using ocean-bottom GPS and deformation data (Ito *et al.*, 2011; Sato *et al.*, 2011) point to a large coseismic slip of more than 60 m near the hypocenter. The occurrence of such a large slip implies a large stress drop associated with the earthquake.

To characterize the earthquake source, we have adopted here a simple approach of waveform inversion based on a point source moment tensor representation using regional broadband strong-motion waveforms. This approach avoids the under-determined problem, and may be used to identify the large stress drop rupture area in a way that is different from previous studies. Our moment-tensor inversion and spectral analysis, based on the omega-square model, point to a localized asperity over a circular fault having a radius of 70 km with an average slip and stress drop of 50 m and 40 MPa, respectively. The stress drop corresponds to an effective normal stress larger than 200 MPa. Such a large effective normal stress is consistent with that inferred from the numerical simulation study of Kato and Yoshida (2011), who suggested the significance of a shallow strong asperity on the occurrence of the Tohoku-Oki earthquake. Yoshida and Kato (2011) explained the large effective normal stress by a pore pressure distribution along the plate. The strong localized asperity may be alternatively explained by a subducted seamount, which increases plate coupling locally (Scholz and Small, 1997). In this paper, we present the results of our analysis of the Tohoku-Oki earthquake, and discuss the origin of the shallow strong asperity.

## 2. Data and Inversion Method

We used broadband strong-motion seismograms from the nationwide broadband seismic network of the F-net, installed and operated by the National Research Institute for Earth Science and Disaster Prevention (NIED) (e.g., Fukuyama *et al.*, 2001). At each F-net station, a velocitytype strong-motion seismometer is installed at the end of a 30–50-m-long vault to record ground velocities up to ±2 m/s.

We used the waveform inversion method developed by Nakano *et al.* (2008), in which the inverse problem was solved in the frequency domain. A double-couple focal mechanism was assumed for a point source in the inversion. A grid search in space was conducted to find the combination of the best-fit fault and slip orientation parameters (strike, dip, and rake angles) and source location. We obtained the moment function in the time domain from the inverse Fourier transform of the frequency components determined by the inversion. The moment function obtained in this way was a band-passed form since we used band-passed observed waveforms for the inversion. A deconvolved form of the moment function was estimated by fitting a function represented by a superposition of elementary functions to a band-passed form of the moment function determined by the inversion.

We used broadband strong-motion records with a sampling frequency of 20 Hz at 10 F-net stations (Fig. 1(a)). The selection of these stations was based on signal-to-noise ratios at low frequencies and to have a wide azimuthal coverage to the source. After instrumental corrections, we applied a band-pass filter between 0.006 and 0.02 Hz and adopted a sampling frequency of 1 Hz. We used a total data length of 512 s starting from 14:46:18 on 11 March, 2011, (Japan standard time) for the inversion. Grid nodes were positioned at horizontal (EW and NS) and vertical intervals of 0.25° and 10 km, respectively (Fig. 1(a)). Green’s functions were calculated with the structure used by routine centroid moment tensor determinations by NIED (Kubo *et al.*, 2002). In the reconstruction of a deconvolved form of the moment function, we used a step-like function as the elementary function, and their time interval, and initial and final times, were determined by the Akaike Information Criterion (see Nakano *et al.* (2008) for details).

## 3. Results

Our waveform inversion indicates that the observed strong-motion waveforms at regional distances are well explained by a point source modeling (Fig. 2). The bestfit source location was estimated at 38.25°N, 143.25°E, at a depth of 30 km, at which the normalized residual was 0.093 (variance reduction of 90.7%). The best-fit focal mechanism was represented by the fault parameters (strike, dip, rake) = (200, 30, 90) (Fig. 1(a)). The estimated mechanism is consistent with those estimated from global broadband seismographic network data by the global CMT project and the National Earthquake Information Center (NEIC) of the U.S. Geological Survey, although the centroid source location and dip angle are slightly different from the global data estimations (Fig. 1(a)). The estimated seismic moment was 4.8 × 10^{22} Nm(*M*_{w} = 9.1) (Fig. 3(a)). The moment-rate function (Fig. 3(b)) shows a source duration of roughly 200 s and a peak moment rate at 50–100 s from the source origin time. Our inversion results indicate that the point source assumption is satisfied in view of the observations at regional distances.

To estimate the source size and the amount of slip, we used the spectra of the observed displacement seismograms at low frequencies, which can be represented by the omega-square model in the far field (Aki, 1967). We estimated the corner frequency of the omega-square model in the following way. A displacement seismogram was corrected for medium attenuation using the following equation: \({u_{\rm{c}}}(\omega) = u(\omega){e^{Bl}}\), where *u* and *u*_{c} are the observed and corrected displacements, respectively; ω is angular frequency; and *l* is the hypocentral distance. Here, *B* is given by \(B = \omega /(2Q{\beta _0})\), where *Q* is the quality factor for medium attenuation and \({\beta _0}\) is an ** S**-wave velocity at shallow depths. We used \({\beta _0} = 3500\) m/s and

*Q =*300. The amplitude spectrum of a corrected displacement seismogram was fitted by the following omega-square model (Aki, 1967): \(S(\omega) = S(0)/[1 + {(\omega /{\omega _{\rm{c}}})^2}]\), where \({\omega _{\rm{c}}} = 2\pi f\) and

*fc*is the corner frequency.

Assuming slip on a circular crack and a rupture velocity of 0.8*β*, where *β* is an *S*-wave velocity at the source, the corner frequency *f*_{c}, for *S* waves of the omega-square model, is related to the crack radius *r* by the equation \({f_{\rm{c}}} = 0.3\beta /r\) (Sato and Hirasawa, 1973). To estimate the corner frequency, we selected stations located at an intermediate distance from the source. This is because seismograms at closer stations may be contaminated by *P* waves and near-field effects and those at distant stations are affected by surface waves. Of the 10 stations used in the waveform inversion, we selected 5 stations (TMR, GJM, KZK, TTO, and JIZ). Since the estimation of the corner frequency is strongly affected by noise, we used additional stations (MMA, SBT, ADM, ASI, ONS, and SGN) (Fig. 1(a)) to obtain a stable estimation. Figures 4(a) and 4(b) show the original and band-passed (0.006-0.02 Hz) vertical velocity seismograms at GJM, respectively. In view of the bandpassed displacement particle motions in Figs. 4(c) and 4(d), the dominant wave recorded in these seismograms is an *SV* wave, which justifies the use of the omega-square model for *S* waves. As shown in Fig. 4(e), the omega-square model reasonably represents the spectrum of the observed data. We estimated *f*_{c} values using the vertical and radial seis-mograms at 11 stations (Fig. 1(a)). The average value of *f*_{c} was 0.016±0.005 Hz. Since the signal-to-noise ratios of aftershocks at low frequencies were poor, the spectral ratio technique could not be applied in this case.

Using *f*_{c} = 0.016 Hz and *β =* 3800 m/s at the source, we obtain \(r \cong 70\;{\rm{km}}\). The rupture duration *τ* for a circular crack rupture including the stopping phase may be given by *τ = 2r*/(0.8β). Using this equation, we obtain \(\tau \cong 40\) s for *r* = 70 km. This duration coincides with the peak pulse duration in the moment-rate function in Fig. 3(b) (orange bar). We therefore conclude that the peak pulse corresponds to the rupture estimated by the corner frequency. The seismic moment for the peak pulse in the moment-rate function is 2.8 × 10^{22} N m, which is 60% of the total seismic moment. The remaining 40% of the seismic moment may correspond to rupture beyond the crack.

The seismic moment *M*_{0} for a circular crack is defined by the equation *M*_{0} = *µAD*, where *µ* is the rigidity, \(A = \pi {r^2}\) is the slip area, and *D* is the average slip. Using *r* = 70 km, *µ =* 40 GPa, and *M*_{0} = 2.8 × 10^{22} N m for the peak pulse, we obtain \(D \cong 50\;{\rm{m}}\). The stress drop Δσ within the crack is estimated to be about 40 MPa following the equation \(\Delta \sigma {\rm{ = (7/16)}}{M_0}/{r^3}\) (Sato and Hirasawa, 1973). This value is anomalously large compared to those of ordinary interplate earthquakes, which are in a range of 1–10 MPa (e.g., Kanamori and Anderson, 1975). The stress drop is given as \(\Delta \sigma = {\sigma _{\rm{i}}} - {\sigma _{\rm{f}}}\), where \({\sigma _{\rm{i}}}\) and \({\sigma _{\rm{f}}}\) are the initial and final shear stresses on the fault, respectively. We define the yield stress \({\sigma _{\rm{s}}} = {\mu _{\rm{s}}}\sigma _{\rm{n}}^{\rm{e}}\), where \({\mu _{\rm{s}}}\) is the static friction coefficient and \(\sigma _{\rm{n}}^{\rm{e}}\) is the effective normal stress, and the dynamic stress \({\sigma _{\rm{d}}} = {\mu _{\rm{d}}}\sigma _{\rm{n}}^{\rm{e}}\), where \({\mu _{\rm{d}}}\) is the dynamic friction coefficient. If we assume that \({\sigma _{\rm{f}}} \cong {\sigma _{\rm{d}}},{\sigma _{\rm{s}}} - {\sigma _{\rm{i}}} = {\sigma _{\rm{i}}} - {\sigma _{\rm{d}}}\), and \({\mu _{\rm{d}}} = 0.5{\mu _{\rm{s}}}\) (Aochi and Kato, 2010), we obtain the relation \(\Delta \sigma = 0.25{\mu _{\rm{s}}}\sigma _{\rm{n}}^{\rm{e}}\). If one assumes \({\mu _{\rm{s}}} = 0.7\) as inferred from laboratory experiments (e.g., Byerlee, 1978), Δσ*=* 40 MPa yields \(\sigma _{\rm{n}}^{\rm{e}}\) = 230 MPa, which is consistent with the effective normal stress inferred by Kato and Yoshida (2011).

## 4. Discussion

Asano *et al.* (2011) has indicated that there exists a region where no aftershocks with thrust focal mechanisms occurred near the source area of the Tohoku-Oki earthquake, and concluded that this region corresponds to the large coseismic slip area. As shown in Fig. 1(b), our estimated asperity size is consistent with this region, which supports our estimation of the rupture size. The Geospatial Information Authority of Japan (GSI) performed a joint slip inversion of co-seismic GPS data from the Japanese nationwide GPS network (GEONET) and at ocean-bottom GPS stations near the epicentral region (Sato *et al.*, 2011). The joint inversion result indicated a localized area \((L \cong 150\;{\rm{km}})\) having a slip larger than 40 m, and a maximum slip of about 60 m near the hypocenter (see http://www.gsi.go.jp/cais/topic110520-index.html). Ito *et al.* (2011) estimated a coseismic slip of roughly 80 m based on ocean-bottom deformation measurements above the source region. Therefore, our seismic estimations of the large slip area \((L = 2r \cong 140\;{\rm{km}})\) and the average slip \((D \cong 50\;{\rm{km}})\) are consistent with these other studies.

Kanamori and Astiz (1985) showed that the ratio *η* of seismic slip to the total plate motion varies systematically as a function of the age of the subducting plate. Values of *η* for subduction zones with relatively young plates are close to 1, but *η* is very small for the northeastern Japan subduction zone, indicating that the plates are almost decoupled. The occurrence of the mega earthquake is apparently not compatible with weak seismic coupling. Our results, indicating a large effective normal stress, imply a strong coupling in the mega asperity.

The estimated large effective normal stress (>200 MPa) is consistent with the numerical simulation study of Kato and Yoshida (2011). They indicated that a strong asperity at a shallow plate interface can reproduce the occurrence of great earthquakes similar to the Tohoku-Oki earthquake. Yoshida and Kato (2011) explained the shallow strong asperity with a pore pressure distribution along the subducted plate. They claimed that the large effective normal stress is achieved by a nearly hydrostatic pore pressure at a shallow part of the plate.

The shallow strong asperity may be alternatively explained by a subducted seamount. Scholz and Small (1997) proposed that subduction of a large seamount increases the normal stress across the subduction interface, which produces local seismic coupling in decoupled plates. The estimated effective normal stress (*>* 200 MPa) may be achieved by a subducted seamount with a base width of 60 km and height of 4 km (typical dimensions of large seamounts) as shown by Schloz and Small (1997).

The two-dimensional model of Kato and Yoshida (2011) does not explain the lateral localization of the asperity. On the other hand, the seamount hypothesis naturally explains the localized asperity and the occurrence of the mega earthquake in the decoupled plates. The tomographic model of Zhao *et al.* (2011) displays velocity anomalies in the source region of the Tohoku-Oki earthquake. Similar velocity anomalies are also seen in the tomographic image of Matsubara and Obara (2011). Both Zhao *et al.* (2011) and Matsubara and Obara (2011) suggested a subducted seamount to be the origin of the velocity anomalies.

On the other hand, no clear structural features indicating a subducted seamount are recognizable in seismic reflection sections along the Japan Trench (e.g., Tsuru *et al.*, 2002). Furthermore, Mochizuki *et al.* (2008) concluded that interplate coupling is weak over a large seamount known as the Daiichi-Kashima Seamount, that is being subducted at the trench off Ibaraki (Fig. 1(b)). Wang and Bilek (2011) suggested that extensive fracturing and faulting in the upper plate accompanied by the uplift due to a subducted seamount provide unfavorable conditions for the generation and propagation of large ruptures. However, the fracturing and faulting may depend on the rheological property of the plate, which was not considered in their study. Further structural investigations and theoretical studies are required to verify the validity of the seamount hypothesis.

In summary, our waveform inversion and spectral analysis, based on the omega-square model, show that the shallow strong localized asperity was ruptured during the Tohoku-Oki earthquake. The pore pressure hypothesis has a difficulty in explaining the localized nature of the asperity, and there is very little supporting evidence for the seamount hypothesis. Future studies are necessary to identify the origin of the shallow strong localized asperity, which is a key to understanding the source process of the Tohoku-Oki earthquake.

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## Acknowledgments

Comments from Nathan Bangs, an anonymous reviewer, and Kiyoshi Yomogida helped to improve the manuscript.

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Kumagai, H., Pulido, N., Fukuyama, E. *et al.* Strong localized asperity of the 2011 Tohoku-Oki earthquake, Japan.
*Earth Planet Sp* **64**, 649–654 (2012). https://doi.org/10.5047/eps.2012.01.004

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DOI: https://doi.org/10.5047/eps.2012.01.004