 Frontier letter
 Open access
 Published:
Swave attenuation structure beneath the northern Izu–Bonin arc
Earth, Planets and Space volume 68, Article number: 55 (2016)
Abstract
To understand temperature structure or magma distribution in the crust and uppermost mantle, it is essential to know their attenuation structure. This study estimated the 3D Swave attenuation structure in the crust and uppermost mantle at the northern Izu–Bonin arc, taking into account the apparent attenuation due to multiple forward scattering. In the uppermost mantle, two areas of high seismic attenuation (high Q ^{−1}) imaged beneath the volcanic front were mostly colocated with lowvelocity anomalies. This coincidence suggests that these highQ ^{−1} areas in lowvelocity zones are the most likely candidates for hightemperature regions beneath volcanoes. The distribution of random inhomogeneities indicated the presence of three anomalies beneath the volcanic front: Two were in highQ ^{−1} areas but the third was in a moderateQ ^{−1} area, indicating a low correlation between random inhomogeneities and Q ^{−1}. All three anomalies of random inhomogeneities were rich in shortwavelength spectra. The most probable interpretation of such spectra is the presence of volcanic rock, which would be related to accumulated magma intrusion during episodes of volcanic activity. Therefore, the different distributions of Q ^{−1} and random inhomogeneities imply that the positions of hot regions in the uppermost mantle beneath this arc have changed temporally; therefore, they may provide important constraints on the evolutionary processes of arc crust and volcanoes.
Background
The Izu–Bonin arc is an intraoceanic island arc on the Philippine Sea plate (Fig. 1). Seismic reflection and refraction surveys have been conducted extensively around this arc to elucidate its crustal structure and evolution processes. An important seismic structure in the Izu–Bonin arc is middle crust (V _{p} = 6.0–6.8 km/s), which was first found by a seismic survey across the volcanic front of the northern arc (Suyehiro et al. 1998). Middle crust is a representative feature of continental crust; therefore, this island arc is considered to be an ideal region for field studies of arc evolution and continental crust generation. Subsequent seismic surveys identified middle crust along many survey lines around this arc and showed that beneath the volcanic front the middle crust tends to be thick beneath basaltic volcanoes (e.g., Kodaira et al. 2007a, b). This clear correlation between volcanoes and crustal structure is a significant constraint on middlecrust generation and arc evolution processes (e.g., Tatsumi et al. 2008).
The uppermost mantle structure beneath this arc is an important boundary condition for evolutionary processes of the volcanoes and crustal structures. Obana et al. (2010) examined the crust and uppermost mantle structures beneath the arc by passive seismic observation with ocean bottom seismographs (OBSs). They focused on the northern part of the Izu–Bonin arc from Hachijojima to Torishima (Fig. 1), where the middle crust beneath the basaltic volcanoes tends to be thicker compared with the southern part (Kodaira et al. 2007b). Their travel time tomography with seismic data of the OBSs and onshore stations revealed several lowvelocity anomalies of P and Swaves in the mantle wedge beneath the volcanic front. These lowvelocity anomalies are presumably related to the magma distribution, but the horizontal extent of these lowvelocity zones was much larger than that of the thick middle crust; therefore, the relationship between these velocity anomalies and the volcano distribution was unclear, in contrast to the clear correlation of the crustal structures with volcanoes.
Another passive seismic imaging in northern Izu–Bonin arc that is an analysis of seismic wave scattering was conducted by Takahashi et al. (2011). They analyzed the Swave envelopes at 4–32 Hz and estimated the spatial variation of the power spectral density function (PSDF) of random velocity inhomogeneities that is a fractional fluctuation of seismic velocity from the average velocity. Their result showed strong inhomogeneities near the volcanic front around the crust (0–30 km depth) and moderately strong inhomogeneities in the uppermost mantle beneath the volcanic front. Correlation of these moderately strong inhomogeneities with the volcano distribution was higher than that of seismic velocity. Their study assumed a PSDF which has powerlaw decay at large wavenumbers to take into account of frequency dependence of scattering and clarified these strong and moderately strong random inhomogeneities were commonly characterized by a gradual spectral gradient. This means that random inhomogeneities beneath the volcanoes are rich in shortwavelength spectra. They suggested that magma intrusions might account for the Swave velocity fluctuations, but this interpretation would not explain the weak correlation with the seismic velocity structure.
In this study, we examined the Swave attenuation tomography of the northern Izu–Bonin arc to elucidate the seismic structure of the crust and uppermost mantle. Seismic wave attenuation in this arc would be an important structural constraint to understand the current magma distribution and temperature structure. For the structure of random inhomogeneities, we used the results reported by Takahashi et al. (2011), and we applied the Swave attenuation tomography method of Takahashi et al. (2014) to the same seismic waveform data used by Takahashi et al. (2011). In this method, the maximum amplitudes at plural frequency bands are analyzed, and the attenuation structures, site amplification factors, and seismic source parameters are estimated simultaneously. The uncertainties of unknown parameters are evaluated by Monte Carlo sampling. In this paper, we outline the method and the seismic data and then describe the attenuation structure beneath the northern Izu–Bonin arc and its uncertainties. Finally, we examine the relations between Q ^{−1} and other seismic structures.
Method
It is assumed that the medium is characterized by random velocity fluctuations and inelasticity. The Swave velocity of the medium on the location x is set to \(V\left( {\mathbf{x}} \right) = V_{0} \left( {1 + \xi \left( {\mathbf{x}} \right)} \right)\), where V _{0} and \(\xi \left( {\mathbf{x}} \right)\) are the background velocity and random fractional fluctuation, respectively. We imagine an ensemble of random media. The ensemble average of the fluctuations \(\xi \left( {\mathbf{x}} \right)\) satisfies \(\left\langle {\xi \left( {\mathbf{x}} \right)} \right\rangle = 0\), where the angle brackets mean the ensemble average. If the characteristic scale of the random inhomogeneities is much larger than the wavelength of the incident wave, multiple forward scattering becomes dominant at large travel distances. Under this condition, envelopes of direct waves can be described by a Markov approximation of the parabolic wave equation (e.g., Sato 1989; Saito et al. 2002). The Markov approximation is a kind of stochastic interpretation of wave scattering in random media that gives the integration of forward scattering processes in thin layers from source to receiver (e.g., Williamson 1972). Takahashi et al. (2011) used this Markov approximation in their estimation of the random inhomogeneity structure in the northern Izu–Bonin arc. Here, we suppose that random inhomogeneities and Q ^{−1} vary in space. By using the Markov approximation, we can calculate the maximum amplitude for an impulsive wavelet radiated from a point source with a unit energy (see Saito et al. 2002 for details) that is equivalent to the scattering attenuation. Then, the Swave maximum amplitude A _{max} of root mean square (RMS) envelope in a narrow frequency band can be written as
at travel distance r and central frequency f. The three components on the righthand side of Eq. (1) are, from left to right, the site effect, the path effect, and the source term.
The \(\rho V_{S}\) is the Swave impedance at the seismic station, where V _{s} and ρ are, respectively, Swave velocity and medium density at a seismic station. S(f), the site amplification factor, is an unknown parameter in our inversion. It represents the local structure effect near a seismic station that cannot be assigned to the Swave impedance or to the path effect. S(f) includes the recording system response and boundary conditions of an OBS or onshore station, as well as the effect of local structure near the seismic station.
The path effect consists of geometrical spreading 1/r, scattering attenuation \(F_{\text{scat}} \left( {r,f,\xi \left( {\mathbf{x}} \right)} \right)\), and the Q ^{−1} effect. The \(F_{\text{scat}} \left( {r,f,\xi \left( {\mathbf{x}} \right)} \right)\) was evaluated for all raypaths and at all frequency bands by a numerical simulation with the Markov approximation (Takahashi et al. 2008). The attenuation factor F _{ Q } is set as
where summation takes place along the raypath, V _{0} is the Swave velocity along the raypath, and \(\varDelta r_{k}\) is the path length of a segment. We assumed the frequency dependence of Q ^{−1} as
where Q ^{−1}_{0} is Q ^{−1} at 1 Hz. Even though parameter γ and its spatial variation were not fully resolved in previous studies of attenuation tomography (e.g., Pozgay et al. 2009), this study set the γ(x) as an unknown parameter with consideration for γ variations in Japan (e.g., Carcole and Sato 2010).
The radiation pattern \(R_{\theta \phi }\) in source term was set to the RMS average of Swave radiation from a point sheardislocation source \(\bar{R}_{\theta \phi } = \sqrt {{2 \mathord{\left/ {\vphantom {2 5}} \right. \kern0pt} 5}}\). Source energy W _{s} is evaluated by using an omegasquare source spectrum model as
where M _{0} and f _{c} are, respectively, the seismic moment and corner frequency and ρ _{0} and β _{0} are the density and Swave velocity, respectively, in the source region (e.g., Kinoshita and Ohike 2002). We selected this source model to reduce the number of unknown parameters.
Unknown parameters in our attenuation tomography are S(f), M _{0}, f _{c}, Q ^{−1}_{0} (x), and γ(x). The study area was partitioned into N blocks that are characterized by Q ^{−1}_{0} and γ. These parameters were estimated by minimizing the misfit and smoothness function s:
The first term is the squared residual of the maximum amplitude A _{max} corrected for the geometrical spreading effect, and the second and third terms are constraint terms for the spatial smoothness of unknown parameters with weighting factors \(w_{{Q_{0} }}\) and \(w_{\gamma }\).
The inversion analysis consists of three steps to achieve a stable estimation of all parameters and a small tradeoff among unknown parameters (Takahashi 2012). The first step estimates the initial model by assuming a spatially uniform attenuation structure: \(Q_{0}^{  1} \left( {\mathbf{x}} \right) = Q_{{0\_{\text{uni}}}}^{  1}\) and \(\gamma \left( {\mathbf{x}} \right) = \gamma_{\text{uni}}\). Only two site factors S(f) are possible during this first step: one for onshore stations and another for OBSs. The second step estimates the Q ^{−1}(x) structure with S(f) under the same constraint as in the first step. The third step refines Q ^{−1}(x) and the source parameters and also estimates S(f) of all stations without any constraints for S(f).
Source parameters were constrained as follows. During the first and second steps, we fixed the M _{0} values of some moderatesized earthquakes by using reference values from the moment tensor catalog, which is routinely published on the Web site of the broadband Fnet seismic network (Okada et al. 2004). We further constrained energy radiation at frequencies higher than f _{c} by assuming Brune’s stress drop (Brune 1970) \(\varDelta \sigma\) = \(\left( {{7 \mathord{\left/ {\vphantom {7 {16}}} \right. \kern0pt} {16}}} \right)\left( {{{M_{0} } \mathord{\left/ {\vphantom {{M_{0} } {\left( {{{2.34\beta_{0} } \mathord{\left/ {\vphantom {{2.34\beta_{0} } {2\pi \, f_{\text{c}} }}} \right. \kern0pt} {2\pi \, f_{\text{c}} }}} \right)}}} \right. \kern0pt} {\left( {{{2.34\beta_{0} } \mathord{\left/ {\vphantom {{2.34\beta_{0} } {2\pi \, f_{\text{c}} }}} \right. \kern0pt} {2\pi \, f_{\text{c}} }}} \right)}}^{3} } \right)\) for the referenced events to be 1 MPa during the first and second steps. Stress drops of other earthquakes were restricted to a narrow range (0.1–10 MPa) during the first and second steps. In the third step, we set a sufficiently wide sampling range of 0.01–100 MPa for all earthquakes. We also set broad sampling ranges for the unknown parameters as follows: 10^{10} Nm < M _{0} < 10^{18} Nm; 10^{−4} < Q ^{−1}_{0} < 10^{−1}; −0.5 < γ < 2.0; and 1/1000 < S(f) < 1000.
Solutions and uncertainties of this inverse problem were evaluated by the exchange Monte Carlo (EMC) method (Hukushima and Nemoto 1996), which is a Markov chain Monte Carlo (MCMC) method. The EMC sets plural temperatures τ _{ i }, (i = 1–n _{ τ }) and generates random number sequences by MCMC for all \(\exp \left( {  {s \mathord{\left/ {\vphantom {s {\tau_{i} }}} \right. \kern0pt} {\tau_{i} }}} \right)\) in parallel. If a sampling point at a higher temperature τ _{ j+1} has smaller s than that at a lower temperature τ _{ j }, the sampling point at τ _{ j+1} will be exchanged with the point at τ _{ j }. The \(\exp \left( {  {s \mathord{\left/ {\vphantom {s {\tau_{i} }}} \right. \kern0pt} {\tau_{i} }}} \right)\) with larger τ _{ i } becomes smooth and gradual and therefore ensures parameter sampling over the whole parameter space. In this study, we set temperatures τ _{ i } as
If we consider the Gaussian likelihood function, uncertainties of unknown parameters are evaluated by the standard deviations of the sampled points at τ _{ i } ≤ 2 \(\sigma^{2}\), where \(\sigma^{2}\) is the variance of \(\log \left( {rA_{\text{max} } } \right)\). This standard deviation is usually called the Monte Carlo standard error. We estimated the optimal solution by taking the ensemble average of the sampled points at τ _{1}, and its variance \(\sigma^{2}\) from the squared residuals of \(\log \left( {rA_{\text{max} } } \right)\) at τ _{1}. These results and errors were evaluated by using 5000 models picked every 100 iterations. This uncertainty reflects the quality and quantity of observed data and therefore would give a clear insight on the reliability of inversion result.
Observations and data
Seismic observation in the northern Izu–Bonin arc (Obana et al. 2010) was conducted from April 2006 to July 2006 with 40 OBSs. Each OBS was equipped with a threecomponent 4.5 Hz seismograph. Waveform data were recorded with a 100 Hz sampling rate. After the observation period, 37 OBSs were recovered, and 36 of these (white squares in Fig. 1) had successfully recorded ground motion. In this area, the National Research Institute for Earth Science and Disaster Prevention (NIED) of Japan (Okada et al. 2004; Obara et al. 2005) operates some seismic stations, two on Hachijojima and one on Aogashima. Seismic data recorded at these stations were also used in this study. Seismic data analysis with both of OBSs and onshore stations detected approximately 4500 earthquakes. Obana et al. (2010) determined the 1D velocity structures of V _{p} and V _{s} and then estimated the initial hypocenter locations using the hypomh program (Hirata and Matsu’ura 1987) before travel time tomography. Following the random inhomogeneity study of Takahashi et al. (2011), we used some of these initial hypocenter locations to estimate the random inhomogeneity structure, and we also referred to the unified hypocenter list provided by the Japan Meteorological Agency (JMA) for events occurring north of the study area (>34.5°N).
The maximum Swave amplitudes were measured from the RMS envelopes at 4–8, 8–16, and 16–32 Hz. RMS envelopes were composed of the horizontal components of the velocity seismograms \(v_{H1} \left( t \right)\) and \(v_{H2} \left( t \right)\) as \(\sqrt {v_{H1}^{2} \left( t \right) + v_{H2}^{2} \left( t \right)}\). We applied the moving average for envelopes in a window whose length was twice the central period. We measured the maximum amplitude in a 30s time window starting from the Swave onset. Examples of observed waveform and envelopes used in this work were shown in Figure 4 in Takahashi et al. (2011). The time window length was manually shortened for the case that large amplitude waves were observed after Swave peak arrival. Some envelopes with no clear peak arrival because of strong scattering or absorption were excluded. Seismograms of these excluded data usually show clear Swave at lower frequency, but weak or no Swave signals at higher frequency. Most of them were the records of backarc side stations. These excluded data suggest existences of high Q ^{−1} or strong inhomogeneity in the backarc, but this information cannot be quantified as attenuation or random inhomogeneity structure.
The earthquakes selected for this analysis occurred near the subducting Pacific plate at 35–300 km depth, and their maximum magnitude was 4.7. The hypocentral distance ranged from 100 to 300 km. These criteria were introduced in the peak delay time analysis of Takahashi et al. (2011) to satisfy some requirements in the Markov approximation. For example, the minimum travel distance was set to secure a sufficient accumulation of multiple forward scattering. Numbers of input data for tomography are 6107 (4–8 Hz), 6138 (8–16 Hz), and 4748 (16–32 Hz). Seismic raypaths were evaluated under the 1D velocity structure used by JMA for the unified hypocenter list (Ueno et al. 2002) as with the study of random inhomogeneities (Takahashi et al. 2011). The study area was divided into 650 blocks, whose dimensions were either 0.60° × 0.60° horizontally × 30 km thick (0–30 km depth) or 0.30° × 0.30° horizontally × 20 km thick (>30 km depth). The number of earthquakes for these data was 651. The number of referenced M _{0} values was 20. We set different impedances for OBSs and island stations. For the OBSs, we used Swave velocity and density values for ocean bottom sediment, V _{s} = 0.15 km/s and ρ = 2.1 g/cm^{3}, taking into account the waveform modeling of OBS data in the northern Izu–Bonin arc (Sato et al. 2009). For the island stations, we used V _{s} = 3.15 km/s and ρ = 2.7 g/cm^{3} (Takahashi et al. 2014). We set V _{0} to 4 km/s, ρ _{0} = 3.2 g/cm^{3} and β _{0} = 4.4 km/s, following Takahashi (2012).
Results
In the first analysis step, uniform Q ^{−1} was estimated to be Q ^{−1}(f) = 10^{−2.8} f ^{−0.68}. This value indicates a relatively weak attenuation of the Swave Q ^{−1} and is similar to the uniform Q ^{−1} estimated in southwestern Japan, Q ^{−1} (f) = 10^{−2.7} f ^{−0.67} (Takahashi et al. 2014).
Weighting factors were selected by considering the Lcurves (Fig. 2a, b) (e.g., Hansen and O’Leary 1993) of the smoothness constraints. The Lcurve is a plot of smoothness constraints against the RMS residual of \(\log \left( {rA_{\text{max} } } \right)\), and it clarifies adequate smoothness for sufficiently small residuals of \(\log \left( {rA_{\text{max} } } \right)\). Although both Lcurves show large scatter, we identified a corner of the Lcurve for γ at \(\log \left( {rA_{\text{max} } } \right)\) = 0.19–0.20 (Fig. 2b, red arrow). The Lcurve for Q ^{−1}_{0} (Fig. 2a) does not show any clear corners, but smoothness tended to increase with decreasing the residual of \(\log \left( {rA_{\text{max} } } \right)\) when the residual was smaller than 0.20–0.22. Here, we assumed an optimal RMS residual of 0.20. With this residual, the smoothness of Q ^{−1}_{0} should be in the range 1.0 × 10^{−4}–1.0 × 10^{−3} and that of γ should be 1.0 × 10^{−4}–1.0 × 10^{−3}. By plotting these smoothness constraints against their weighting factors (Fig. 2c, d), we inferred that both \(w_{{Q_{0} }}\) and \(w_{\gamma }\) should be 5.0 × 10^{3}–1.0 × 10^{4}; thus, we selected \(w_{{Q_{0} }}\) = 1.0 × 10^{4} and \(w_{\gamma }\) = 1.0 × 10^{4}. Using these weighting factors, we evaluated the Monte Carlo standard errors by using samples at \(\tau_{1}\tau_{9}\) (\(\tau_{9}=0.0816\)); here, \(\tau_{9}\) is close to 2 \(\sigma^{2}\) (~0.08). Note that large scatter of Lcurve is due to mutual interaction between \(w_{{Q_{0} }}\) and \(w_{\gamma }\). For example, if \(w_{\gamma }\) is set in a narrow range near the optimal value, the Lcurve for γ shows smaller scatter.
We next examined the relationship between the source parameters M _{0} and f _{c} (Fig. 3). Most of the estimated M _{0} were distributed in a narrow range from 10^{12} to 10^{14} Nm. The smallest M _{0} of the referenced events was 2.26 × 10^{14} Nm. M _{0} of unreferenced events would be smaller than this minimal moment; therefore, this moment range seems reasonable. Stress drop was scattered around 1–10 MPa. This stress drop tends to be larger than that reported by previous studies (e.g., Takahashi et al. 2014), but larger stressdrop events tend to show larger Monte Carlo standard errors of f _{c}. A possible origin of larger uncertainty for higher f _{c} is small number of data at the highest frequency band (16–32 Hz), since accurate estimation of higher f _{c} requires seismic data at higher frequency.
The site factor S(f) (Fig. 4a) generally decreased with increasing frequency, and S(f) in each frequency band was distributed randomly in space without any systematic trend. The Monte Carlo standard errors (Fig. 4b) were generally small, with some exceptions. The large error in the backarc side at 16–32 Hz was probably due to the small number of data. Except at this station, site amplification factors were distributed from 0.04 to 2.3. The decreasing S(f) with increasing frequency can be interpreted to mean that Q ^{−1} in the sediment layer beneath the seafloor was frequency independent or only weakly frequency dependent. Most site factors were less than 1.0, which means that attenuation occurred in the vicinity of seismic stations. The small site amplification factors may mean that the assumed impedances at the seismic stations were smaller than the true values.
The 3D attenuation structures and the Monte Carlo standard errors are shown in map views of the results at 0–30, 30–50, and 50–70 km depths (Figs. 5, 6, 7). Figure 5 shows Q ^{−1}_{0} and γ, and their Monte Carlo standard errors; for each depth interval, Figs. 6 and 7 show Q ^{−1} values and their Monte Carlo standard errors, respectively, at 4–8, 8–16, and 16–32 Hz. Q ^{−1} values were calculated from the estimated Q ^{−1}_{0} and γ on the basis of a simple relation (Eq. 3). Examination of these Q ^{−1} maps can give intuitive insights into the attenuation structures. By applying the Born approximation to the random inhomogeneities in this area as with Takahashi (2012), we confirmed that Q ^{−1} of backscattering was less than 3 % of the estimated Q ^{−1} in the study area. Thus, we consider the estimated Q ^{−1} to mainly reflect the inelasticity of medium.
At 0–30 km depth, both Q ^{−1}_{0} and γ showed clear differences between the northern and southern parts of the study area, but Q ^{−1} was nearly constant. The Monte Carlo standard error of Q ^{−1} was large only on the forearc side. This large error was due mainly to the large uncertainty of Q ^{−1}_{0} . We note that inversion results with smaller \(w_{{Q_{0} }}\) and \(w_{\gamma }\) frequently showed lower Q ^{−1} on the forearc side than on the backarc side. Therefore, our data may contain information on the E–W variation of Q ^{−1} in this depth range, but there is not enough information in our data to resolve such horizontal variation. Although the N–S variations of Q ^{−1}_{0} and γ should be reliable, it is difficult to infer their possible origins because they show no clear correlation with other seismic structures.
At 30–50 and 50–70 km depth, Q ^{−1} showed clear variations between the area east and west of the volcanic front. At 4–8 Hz, Q ^{−1} was about 10^{−2.3}–10^{−2.5} in highQ ^{−1} areas (A, B, C and D in Fig. 6) and ~10^{−3.2} at most on the forearc side. In both the northern and southern parts of the study area, the standard errors of Q ^{−1}_{0} were larger on the forearc side. Because the number of data on the forearc side was larger than that on the backarc side, the larger errors may reflect the uncertainties of the hypocenter locations outside the network. At 30–50 km depth, we recognized two highQ ^{−1} areas beneath the volcanic front. One is the areaA beneath Hachijojima and another is areaB beneath Torishima. The Q ^{−1} values in both highQ ^{−1} areas are up to 10^{−2.50} at 8–16 Hz. The Monte Carlo standard errors showed that this alongarc variation is reliable. Note that results with smaller weights (\(w_{{Q_{0} }}\) = \(w_{\gamma }\) = 1.0 × 10^{3}) showed third highQ ^{−1} (~10^{−2.5} at 8–16 Hz) anomaly on the backarc side of Sumisujima. However, this anomaly was not significant due to large uncertainty. At 50–70 km depth, two highQ ^{−1} areas were also imaged beneath the volcanic front at areas C and D. Q ^{−1} at 8–16 Hz in C and D are up to 10^{−2.28} and 10^{−2.47}, respectively. They are at different locations from the highQ ^{−1} areas (A and B) at 30–50 km depth. North of Hachijojima at 50–70 km depth, however, Q ^{−1} showed large uncertainties. Therefore, the meaningful difference between Q ^{−1} in these two depth intervals is the width of the lowQ ^{−1} area between the two highQ ^{−1} areas. We also recognized moderately highQ ^{−1} areas in the north and south on the forearc side (E and F in Fig. 6) that is the most evident at 4–8 Hz. Q ^{−1} in the northern anomaly is 10^{−3.0} at 4–8 Hz, and that in southern anomaly is up to 10^{−2.75} at 4–8 Hz. The anomaly in the northern part was not significant owing to the large uncertainty, but the southern anomaly is worth discussing.
Discussion
Alongarc variation of Q ^{−1} was clearly imaged in the uppermost mantle at 30–50 km depth beneath the volcanic front. However, its correlation with the volcano distribution was not high because of the large horizontal extent of the highQ ^{−1} areas. The seismic velocity structure (Obana et al. 2010) shows two lowVs anomalies at 30–70 km depth beneath the volcanic front: One is north of Aogashima and the other is south of Sumisujima. Most of the highQ ^{−1} areas at 30–50 and 50–70 km depth are within these lowVs areas, and lower Q ^{−1} beneath the volcanic front was imaged between Aogashima and Sumisujima (Fig. 8). Accordingly, lowVs and high Q ^{−1} were mostly correlated in this arc. According to laboratory experiments, \(\log Q^{  1}\) can be represented as \(\log Q^{  1} = \gamma \left( {X  {Y \mathord{\left/ {\vphantom {Y T}} \right. \kern0pt} T}} \right)\), where X and Y (>0) are parameters related to rock properties and pressure and T is medium temperature (e.g., Karato and Jung 1998; Behn et al. 2009). In this entire study area, γ was positive, and γ in highQ ^{−1} areas tended to be smaller than on the forearc side. Although this horizontal variation of γ means that high Q ^{−1} beneath volcanoes did not necessarily correspond to high temperatures, γ showed very weak variation near ToriShima. This result suggests that the high Q ^{−1} beneath Torishima (areaB) at 30–50 km depth is probably an indicator of higher temperature there than on the forearc side, and the moderate Q ^{−1} between Hachijojima and Torishima likely means lower temperatures than in the Torishima area. The highQ ^{−1} area in the lowvelocity anomaly beneath Hachijojima may indicate high temperature, as in ToriShima area, but because of the small γ there, we cannot be certain. It is reasonable to infer that highQ ^{−1} and lowvelocity areas are the most likely candidates for hightemperature areas, but this possibility can only be confirmed by a detailed examination with suitable values for X and Y beneath Hachijojima. Tamura et al. (2002) hypothesized hot fingers of the mantle wedge were present in northeastern Japan, on the basis of the correlation between seismic velocity in the mantle wedge and the Quaternary volcano distribution. In the northern Izu–Bonin arc, we therefore might expect two hot regions in the uppermost mantle to be located in the highQ ^{−1} areas.
Anomalies of random inhomogeneities at 30–70 km depth in Takahashi et al. (2011) were imaged beneath Hachijojima, the Aogashima–Sumisujima area, and Torishima. This random inhomogeneity structure was estimated by assuming the von Kármán type power spectral density function (PSDF) \(P\left( m \right) = {{8\pi^{{{3 \mathord{\left/ {\vphantom {3 2}} \right. \kern0pt} 2}}} \varepsilon^{2} a^{3} \, \varGamma \left( {\kappa + {3 \mathord{\left/ {\vphantom {3 2}} \right. \kern0pt} 2}} \right)\left( {1 + a^{2} m^{2} } \right)^{{  \left( {\kappa + {3 \mathord{\left/ {\vphantom {3 2}} \right. \kern0pt} 2}} \right)}} } \mathord{\left/ {\vphantom {{8\pi^{{{3 \mathord{\left/ {\vphantom {3 2}} \right. \kern0pt} 2}}} \varepsilon^{2} a^{3} \, \varGamma \left( {\kappa + {3 \mathord{\left/ {\vphantom {3 2}} \right. \kern0pt} 2}} \right)\left( {1 + a^{2} m^{2} } \right)^{{  \left( {\kappa + {3 \mathord{\left/ {\vphantom {3 2}} \right. \kern0pt} 2}} \right)}} } {\varGamma \left( \kappa \right)}}} \right. \kern0pt} {\varGamma \left( \kappa \right)}}\), where γ is the gamma function, m is the wavenumber in space, and parameters a, ε, and κ are, respectively, the correlation distance, the root mean square of fractional fluctuation, and a parameter related to the spectral gradient at large wavenumbers (m ≫ 1/a). The three anomalous random inhomogeneities were commonly characterized by smaller κ (Fig. 8a) and in these areas P(m) at large wavenumbers were moderately large compared with the surrounding areas. In these small κ areas, random inhomogeneities are rich in shortwavelength spectra. Takahashi et al. (2011) interpreted these moderately strong inhomogeneities to reflect magma inclusions, because fluid magma can cause large Swave velocity fluctuations. However, recent studies in southwestern Japan (Takahashi et al. 2013, 2014) have shown that strong inhomogeneities with a gradual spectral gradient show high spatial correlations with volcanic rock areas rather than with the Quaternary volcano distribution and that the attenuation structure in southwestern Japan seems to be related to magma and fluid distributions. Therefore, the three areas of anomalies of random inhomogeneities in the uppermost mantle reflect the accumulated intrusions of volcanic rocks during volcanic activity, whereas highQ ^{−1} areas probably reflect the current magma distribution or hightemperature regions. The accumulated volcanic processes would be more relevant to the generation of arc volcanoes and continental crust in this arc. We have already inferred the presence of two hot regions in highQ ^{−1} areas in the uppermost mantle. However, we may need to consider three hot regions at the top of uppermost mantle to describe the arc evolution and volcano distribution. Tamura et al. (2009) suggested that horizontal dykes in the crust could explain small spatialscale variation of the middle crust on the basis of crustal structures, seismic reflectors, and petrological information. Our interpretation of the random inhomogeneities suggests the importance of volcanic processes in the current lowQ ^{−1} area in the uppermost mantle.
The forearc side of the mantle wedge showed moderately highQ ^{−1} areas at 30–50 km depth at areas E and F. Taking into account the uncertainty, only the anomaly in the south (areaE) is meaningful. Travel time tomography imaged some small lowV _{p} and lowV _{ s } anomalies on the forearc side of the volcanic front, 50 km east of Aogashima, Sumisujima, and Torishima in the crust and uppermost mantle (Fig. 9 in Obana et al. 2010). They argued that the anomalies were related to the frontal arc high, which is a remnant Oligocene arc. Our moderately highQ ^{−1} area included only one lowvelocity anomaly, east of Torishima. Therefore, the results of the present study suggest that this Q ^{−1} anomaly is not necessarily due to the remnant arc. The east side of this moderately highQ ^{−1} area is in the subducting Pacific plate, and Q ^{−1} at 16–32 Hz showed a slight increase on the eastern side of this Q ^{−1} anomaly. Even though this increase of Q ^{−1} may not be significant given the uncertainties, it is possible that this moderately high Q ^{−1} was artificially generated by connecting the highQ ^{−1} area beneath Torishima with one in the subducting slab. If a Q ^{−1} anomaly exists in the subducting slab in this area, it would have important implications for studies on fluid transportation and arc magmatism beneath this arc. In southwestern Japan, slight increases of Q ^{−1} were found near the top of the subducting slab (Takahashi et al. 2014). Even though the spatial resolution was too low for a detailed examination, Q ^{−1} would be a sensitive indicator of fluid distribution in the subducting plate when we remove the apparent attenuation effect due to multiple scattering. Studies of Q ^{−1} using data from OBSs near the trench axis or on the incoming plate would clarify possible origins of Q ^{−1} near the subducting plate.
Conclusion
This study estimated the Q ^{−1} attenuation structure in the northern Izu–Bonin arc, taking into consideration the apparent amplitude attenuation due to random velocity inhomogeneities. At 0–30 km depth, the inversion result showed large Monte Carlo standard errors on the forearc side, which prevented horizontal variations of Q ^{−1} from being resolved. Meanwhile, at 30–70 km depth, we clearly imaged some anomalies of high and moderate Q ^{−1} beneath the volcanic front and in the forearc side. Beneath the volcanic front, two highQ ^{−1} zones were almost colocated with lowvelocity anomalies. These highQ ^{−1} areas are the most likely candidates for hightemperature regions beneath the volcanoes. The studies on wave scattering had reported that random inhomogeneities showed three anomalies at 30–70 km depth beneath the volcanic front (Takahashi et al. 2011). All of these anomalies of random inhomogeneities were characterized by a gradual spectral gradient of power spectral density at large wavenumber. If we consider relatively high correlation between such random inhomogeneity with gradual spectral gradient and igneous rock area that is recently pointed out in the southwestern Japan (Takahashi et al. 2013), the most probable interpretation of such spectra is the existence of volcanic rock, related to the accumulated magma intruded during episodes of volcanic activity. Therefore, the different distributions of Q ^{−1} and random inhomogeneities imply temporal changes of volcanic activity in this arc.
Abbreviations
 OBS:

Ocean bottom seismograph
 PSDF:

Power spectral density function
 RMS:

Root mean square
 EMC:

Exchange Monte Carlo
 MCMC:

Markov chain Monte Carlo
 JMA:

Japan Meteorological Agency
 NIED:

National Research Institute for Earth Science and Disaster Prevention
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Authors’ contributions
TT estimated and interpreted the Q ^{−1} structure and drafted the paper with contributions from all coauthors. KO participated in data acquisition as a chief scientist. SK organized the dataacquisition cruises and participated in the interpretation. All authors contributed to scientific discussions. All authors read and approved the final manuscript.
Acknowledgements
This work was partially supported by GrantinAid for Young Scientists (B) (20740261) and GrantinAid for Scientific Research (B) (20340122). We thank those at NIED involved in the development and ongoing maintenance of the Hinet and Fnet systems. Generic Mapping Tools software (Wessel and Smith 1998) was used to produce the figures presented here, and Seismic Analysis Code software (Goldstein et al. 2003) was used for signal processing.
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The authors declare that they have no competing interests.
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Takahashi, T., Obana, K. & Kodaira, S. Swave attenuation structure beneath the northern Izu–Bonin arc. Earth Planet Sp 68, 55 (2016). https://doi.org/10.1186/s4062301604313
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DOI: https://doi.org/10.1186/s4062301604313