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# Rapid magnitude determination from peak amplitudes at local stations

*Earth, Planets and Space*
**volume 65**, pages 843–853 (2013)

## Abstract

The rapid determination of its magnitude soon after a great earthquake is necessary for the issuing of effective tsunami warnings, as demonstrated in the great earthquake off Tohoku district in Japan on March 11, 2011. The earthquake magnitude for the first tsunami warning was underestimated due to magnitude saturation. This paper proposes a method to determine magnitude rapidly from peak velocity and displacement of long-period seismic waves up to 100 seconds at local stations. When waveform data at local stations are available, the magnitude from *S*-wave peaks is expected to be determined faster than that from only *P*-wave peaks. It takes about 140 seconds to estimate a magnitude of about 9 for the March 11, 2011, earthquake, which would enable us to issue the first tsunami warning within three minutes after the same type of earthquake.

## 1. Introduction

The displacement magnitude determined by the Japan Meteorological Agency (JMA) (Katsumata, 2004) indicated saturation during the 2011 off the Pacific coast of Tohoku Earthquake on March 11 of *M*_{w} 9.0 (Hirose et al., 2011). Magnitude determination is a key to issuing an effective tsunami warning. The JMA displacement magnitude is determined from the logarithm of the maximum displacement amplitude recorded with seismographs of natural period 6 s and damping coefficient of 0.55. Displacement records are currently obtained from acceleration records by numerical integration and digital filtering. Using longer-period seismic waves for magnitude determination should overcome the problem of magnitude saturation (Aki, 1967). Here, we use the peak velocity and displacement of a longer period than that used for the JMA magnitude to rapidly determine the magnitude.

Several magnitude determination methods have been proposed for a tsunami warning based on *P*-wave before the *S*-wave arrival (Tsuboi et al., 1995; Yoshida, 1995; Hara, 2007; Kanamori and Rivera, 2008; Lomax and Michelini, 2009). When the fault rupture lasts a long time, the epicen-tral distance of data should be great enough to get a *T*_{
S
} −*T*_{
P
} exceeding the rupture duration, where *T*_{
p
} and *T*_{
S
} are the travel times of *P* and *S* waves.

The broken curve in Fig. 1 indicates the time when the *P*-wave magnitude can be determined. The time is considered to be the sum of the *P*-wave travel time and the source duration of the earthquake. The source duration of an earthquake is assumed to be sixty seconds in the figure. Since the *S*-wave amplitude often exceeds the *P*-wave amplitude, the *P*-wave magnitude should be determined from the data before the *S*-arrival. The *T*_{
S
} − *T*_{
p
} time should exceed the source duration (*D*) for the *P*-wave magnitude. The range of *T*_{
S
} − *T*_{
p
} < *D* is not shown in the figure. The solid curve in the figure denotes *T*_{
S
} + *D*, which is the time when the *S*-wave magnitude can be determined. When data at local stations are available, the magnitude can be determined more quickly from the amplitude of *S*-waves than from that of only *P*-waves.

Quick magnitude determination methods have been proposed also for early earthquake warning (Wu et al., 1998; Kamigaichi, 2004; Wu and Zhao, 2006; Zollo et al., 2006). However, those methods are based on the amplitude measured on waveforms of intermediate period, or the amplitude of the initial parts after the onsets, and do not fit magnitude determination for great and long source duration earthquakes.

For the *P*-wave magnitude determination, it is necessary to restrict the amplitude search range within *P*- and *S*-arrivals to avoid *S*-wave contamination. When any phase type indicating the peak amplitude can be used, time windows for the amplitude search are not needed. This makes the process flow simple and robust. Here, we examine the magnitude determined from the peak amplitude of any phases including long-period *S*-waves and surface waves.

## 2. Method and Data

The peak velocity (m/s) or displacement (m) *A* and magnitude *M* are assumed to be expressed as follows:

Here, *a, b*, and *c* are constants, and *R* (km) is the hypocen-tral distance. *A* is measured over a seismic record on a vertical component obtained at a local station. A dip slip along a plate boundary may cause a large tsunami, and is expected to generate large *P-SV* mode seismic waves, which appear on the vertical component.

Velocity and displacement records are obtained from strong-motion acceleration records with numerical integration and low-cut filters. Second- (for velocity) and Third-(for displacement) order low-cut Bessel filters (Katsumata, 1993) are used in this study. The filters are recursive, and can be applied in real-time processing.

Several cutoff periods are used to measure *A*. Cutoff periods of low-cut filters are set at 1, 2, 5, 10, 20, 50, and 100 seconds. Various cutoff periods (*T*_{
c
}) are used to accommodate a broard range of magnitudes. Examples of waveforms are presented in Fig. 2. Constants *a*, *b* and *c* are estimated so as to minimize the difference between *M* in Eq. (1) and *M*_{w} of the Global CMT solutions. The constants in Eq. (1) are estimated for velocity/displacement and each cutoff period. We assume a common value of *a* for all *T*_{
c
} in Eq. (1), since we expect to see magnitude saturation in the result. The values of *b* and *c* are estimated for each *T*_{
c
}, individually.

Parameter *a* is first estimated with data of earthquakes *M*_{w} > 7, then *b* and *c* are estimated with data including those of smaller events. When the constants *a, b*, and *c* are estimated simultaneously, *M* of great earthquakes (*M*_{w} > 8) diverges further from *M*_{w}. We adopt the value of *a* for a *T*_{
c
} which indicates the least dispersion for earthquakes including small ones, since such a value would be applicable to great earthquakes as well as to moderate ones.

The acceleration records were obtained with a seismic network installed by JMA. The station map is presented in Fig. 3. The accelerometers record ground motion up to ±3 G with a resolution of 0.5 × 10^{−5} m/s^{2} (Japan Meteorological Agency, 2011), which corresponds to a 22-bit resolution. We use only velocity and displacement amplitudes that exceed 0.5 × 10^{−5}/(2*π*/*T*_{
c
}) m/s and 0.5 × 10^{−5}/(2*π*/*T*_{
c
})^{2} m.

Records of fifty-five earthquakes of *M*_{w} > 6.0 from 2001 to 2011 are used. The epicenter map of the earthquakes is presented in Fig. 4.

## 3. Results

Tables 1 and 2 list the obtained values of coefficients *a*, *b* and *c* for the magnitude determination. We adopted the estimated *a* for the cutoff period of fifty seconds, since it provided the smallest standard deviation for earthquakes, including smaller ones than those used for estimating *a* (*M*_{w} > 7). The coefficient for the amplitude *a* in Eq. (1) is greater for velocity than for displacement. This relationship has been seen previously for short-period amplitude measurements (Watanabe, 1971; Katsumata, 2001).

Figures 5 and 6 present data plots with the fitted lines. The relationship between hypocentral distance and amplitude depends on the cutoff periods: the shorter the cutoff period, the steeper the attenuation. The displacement amplitude attenuation depends more on the cutoff period than does the velocity amplitude. The dependence on the period would be related to inelastic attenuation and the seismic wave type that exhibits a peak amplitude. Data deviates from the fitted line at short epicentral distances. The dispersion of log_{10}*A* ranges from 0.22^{2} to 0.33^{2} for the velocity magnitude, and from 0.21^{2} to 0.34^{2} for the displacement magnitude. Amplitude data of velocity and displacement have similar data dispersions.

Figures 7 and 8 illustrate the relationship between the moment magnitude *M*_{w} and the difference of the estimated magnitude *M* (Eq. (1)) from *M*_{w}. Since a common value of *a* is used in Eq. (1), magnitude saturation is seen in shorter cutoff periods (Figs. 7 and 8). Standard deviations of *M* − *M*_{w} range from 0.18 (*T*_{
c
} = 100 s) to 0.32 (*T*_{
c
} = 1 s) for velocity magnitude and from 0.15 (*T*_{
c
} = 100 s) to 0.27 (*T*_{
c
} = 1 s) for displacement magnitude. Deviations of velocity magnitudes are slightly larger than those of displacement magnitudes.

## 4. Discussion

### 4.1 Velocity magnitude and displacement magnitude

In this section, we will briefly discuss the suitability for tsunami warning of velocity and displacement magnitudes. Dispersion of data (Figs. 5 and 6) and differences from *M*_{w} (Figs. 7 and 8) do not clearly differ between velocity and displacement magnitudes. Data from accelerometers are used here with numerical integration, and data availability is limited by *a*_{
r
} /*ω* for velocity and *a*_{
r
} /*ω*^{2} for displacement, where *a*_{
r
} is the sensor resolution of the accelerometer and *ω* is the angular frequency. Velocity magnitude is available for more events due to the limitation on the amplitude range.

For tsunami earthquakes such as the 1992 Nicaragua earthquake (Kanamori and Kikuchi, 1993), the low-frequency component is more dominant than in normal earthquakes. The displacement magnitude is more sensitive to the low-frequency component than is the velocity magnitude. The displacement magnitude is thus preferable for tsunami warnings. The displacement magnitude is mainly examined in the following sections.

The integral of displacement is proportional to the seismic moment, and this might be better for tsunami warning than the displacement amplitude. However, accelerometers do not have enough resolution for more integration. When data of strong motion velocity meters are used for the same purpose, a longer-period component could be used. Since accelerometer networks are more dense than strong motion velocity meter networks, we use accelerometer data in this study.

### 4.2 Application to rapid magnitude determination

The proposed magnitude is considered to be used to observe the growth of magnitude value in real-time processing. Since recursive filters are used to obtain the velocity/displacement records and the transmission and processing delay could be no more than several seconds, it is possible to see the magnitude value change soon after the hypocenter determination. Because they are not used, inversion analysis and phase identification do not introduce additional delay.

The proposed magnitude determination method is applied to some large earthquakes, and the results are presented in Fig. 9. The horizontal axis in the figure represents time from the earthquake occurrence. The magnitude is determined from maximum amplitudes measured until the time indicated on the horizontal axis at the closest three to ten stations. The magnitude value changes with the arrivals of larger seismic waves. It reaches a stable value when peak amplitudes are observed at all of the closest ten stations. The epicenters of the events in Fig. 9 are labeled (a)–(e). Event (f) is an earthquake off the coast of Chile in 2010. Data obtained by the University of Chile are used for event (f).

For the 2011 off the Pacific coast of Tohoku earthquake, the magnitude reached the final value within 140 seconds. The target time of the first tsunami warning in JMA is three minutes, so 140 seconds is a satisfactory time for the first tsunami warning. The final magnitude was 8.8 in the figure, which is less than *M*_{w} 9.1.

The time to reach the final magnitude of other earthquakes is less than three minutes. The times are delayed for events with epicenters far from the closest stations such as earthquakes off the Kuril Islands. However, tsunami arrivals at the nearest coasts would also be delayed for those earthquakes.

As expected, magnitude saturation is observed in Fig. 9. Magnitudes of shorter cutoff periods are generally smaller than those of longer cutoff periods. Differences among M20, *M*_{50} and *M*_{100} are not so large, but the difference between *M*_{10} and *M*_{20} is relatively large (the subscript denotes the cutoff period). Two large pulsed peaks with widths of about twenty seconds are seen in the seismic records in Fig. 2. The asperity size and its slip process would have defined the pulse width which is related to the characteristics of the magnitude saturation. The similarity of *M*_{20}, *M*_{50} and *M*_{100} might be related to fault-rupture characteristics of the regions.

For the 2010 Chile event, short-period magnitudes are greater than long-period magnitudes. This reversed magnitude relationship would be related to the concentrated distribution of the used stations in the northern region of the source area, the relatively southern location of the epicenter, and a large slip in the northern area (Lay et al., 2010). Since the amplitude decay is steeper in short-period magnitudes than in long-period magnitudes (Fig. 6), the uneven station distribution and the improper assumption of the distance to the source affect the short-period magnitudes more. Even in such a case, the long-period magnitude is considered to be more reliable than the short-period magnitude.

The time to reach the final value and the final magnitude depend on the station distribution and the upper limit of station numbers. Figure 10 presents variations of estimated magnitudes with the period from the event origin time for various upper limits of station numbers for the 2011 off the Pacific coast of Tohoku earthquake. As expected, the magnitude reaches the final value earlier for fewer upper limit stations. However, the time difference in reaching the final value is not large in Fig. 10. The final magnitude increases with more stations, and approaches *M*_{w} (9.1). No large difference in dispersion is seen. The upper limit station number can be set arbitrarily, and could be determined based on the required time limit and the difference from the final value.

The magnitudes obtained in this study are compared with Mwp (Tsuboi et al., 1995; Whitmore et al., 2002) in Fig. 11 for the 2011 off the Pacific coast of Tohoku earthquake. Station magnitudes are shown in the figure with the time when the peak amplitudes were measured on the horizontal axis. A short peak-time generally means a short epicen-tral distance. Both magnitudes are determined from data of strong motion velocity meters installed by the National Research Institute for Earth Science and Disaster Prevention. The instrumental response is corrected with the recursive deconvolution filter proposed by Kanamori and Rivera (2008). Since the seismic wave for *M*_{wp} is restricted to the period between *P* and *S* arrivals, and *T*_{
S
} − *T*_{
p
} at a station of short epicentral distance is less than the source duration, the resultant *M*_{wp} at a close station is much less than the moment magnitude of the event (*M*_{w} 9.1). *M*_{wp} at stations become stable after about four minutes from the event origin time. On the other hand, the magnitude of this study scatter around the magnitude 9 even at close stations. However, the station magnitude scatter of this study seems to be larger than that of *M*_{wp}.

### 4.3 Effect of fault type

Events of the same size with a different focal mechanism radiate seismic waves of different amplitude. The amplitude difference due to the fault type is investigated with synthetic records, and the results for dip and strike slip events are shown in Fig. 12. The synthetic records are calculated with the method of Takeo (1985), assuming a velocity structure in Table 3, a focal depth of 20 km, and a triangle source time function of sixty second duration. A high-pass filter of 100-s cutoff is applied to the records.

The amplitude reduces considerably when the station is located in the direction of the nodal planes. Since the compression/tension axis is usually oriented normal to the trench axis for events around a convergent plate boundary and the stations are installed in inland areas, it is considered that the observed amplitude would not become so small for local events. When seismic waves from events near Kuril Islands are observed on the Japan Islands, the stations are distributed around the direction of the null axis of the events and the magnitude would be underestimated. For the strikeslip event, the averaged amplitude is a little smaller (×0.8) than that for the dip-slip event in Fig. 12.

### 4.4 Dependence on the epicenter location

The source region of the 2011 off the Pacific coast of Tohoku earthquake extended about 450 km (Yoshida et al., 2011). An earthquake of a different epicenter might have a similar size of source region. Different epicenters are assumed for the magnitude determination. Figure 13 presents magnitude differences for different epicenters for a 100-s cutoff period. Data acquired at the closest ten stations are used. The reference magnitude is that for the estimated hypocenter (the cross in the figure). The epicenters are assumed to be within the 5-m-slip contour of Yoshida et al. (2011). The magnitude difference is less than 0.25 of the magnitude unit. The difference does not exceed 0.1 over a large part of the area, so the magnitude difference is not significant.

The difference is greater for magnitudes of shorter periods due to high amplitude decay rates of short-period magnitudes (Fig. 5).

## 5. Conclusions

A rapid magnitude determination method for tsunami warning based on the peak velocity and displacement of long-period seismic waves is presented. Cutoff periods up to 100 seconds were used to obtain the seismic wave data from acceleration records. The magnitude did not saturate up to magnitude 9 and could be determined within three minutes for the great earthquake on March 11, 2011, off the Tohoku District, Japan.

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## Acknowledgments

We used data obtained by the Japan Meteorological Agency, University of Chile, and National Research Institute for Earth Science and Disaster Prevention. We used programs developed by Dr. Takeo to calculate synthetic records. We greatly appreciate kind and thoughtful comments from two anonymous reviewers. This study was partly supported by the SATREPS project of “Enhancement of technology to develop tsunami-resilient community”.

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### Cite this article

Katsumata, A., Ueno, H., Aoki, S. *et al.* Rapid magnitude determination from peak amplitudes at local stations.
*Earth Planet Sp* **65, **843–853 (2013). https://doi.org/10.5047/eps.2013.03.006

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DOI: https://doi.org/10.5047/eps.2013.03.006

### Key words

- Magnitude determination
- tsunami warning
- long-period seismic wave
- great earthquakes