Seismic imaging and velocity structure around the JFAST drill site in the Japan Trench: low V p, high V p/V s in the transparent frontal prism

Abstract

Seismic image and velocity models were obtained from a newly conducted seismic survey around the Integrated Ocean Drilling Program (IODP) Japan Trench Fast Drilling Project (JFAST) drill site in the Japan Trench. Pre-stack depth migration (PSDM) analysis was applied to the multichannel seismic reflection data to produce an accurate depth seismic profile together with a P wave velocity model along a line that crosses the JFAST site location. The seismic profile images the subduction zone at a regional scale. The frontal prism where the drill site is located corresponds to a typically seismically transparent (or chaotic) zone with several landward-dipping semi-continuous reflections. The boundary between the Cretaceous backstop and the frontal prism is marked by a prominent landward-dipping reflection. The P wave velocity model derived from the PSDM analysis shows low velocity in the frontal prism and velocity reversal across the backstop interface. The PSDM velocity model around the drill site is similar to the P wave velocity model calculated from the ocean bottom seismograph (OBS) data and agrees with the P wave velocities measured from the core experiments. The average V p/V s in the hanging wall sediments around the drill site, as derived from OBS data, is significantly larger than that obtained from core sample measurements.

Background

The 2011 Tohoku earthquake occurred along the Japan Trench subduction zone east off the northern Honshu island, Japan. The earthquake rupture likely propagated along the plate boundary up to the trench axis. (e.g., Ide et al. 2011; Kodaira et al. 2012). Rapid response drilling by the Integrated Ocean Drilling Program (IODP) Expedition 343 (Japan Trench Fast Drilling Project (JFAST)) successfully drilled through the inferred plate boundary fault approximately 6 km landward of the trench axis. The expedition obtained logging data and core samples, and installed and recovered temperature sensors (Chester et al. 2012). The drilled plate boundary fault is very thin (<5 m) and localized in a pelagic clay layer approximately 15 m above the basal chert layer (Chester et al. 2013). Borehole breakout orientations indicate the stress state of the hanging wall is in normal fault regime and a complete stress drop occurred during the earthquake (Lin et al. 2013). The temperature observatory recorded a residual co-seismic frictional heat anomaly at the plate boundary (Fulton et al. 2013) and estimated a low friction coefficient (<0.1) that is consistent with values from high-speed friction experiments on the fault core sample (Ujiie et al. 2013). All of these results support the hypothesis that co-seismic slip extended to the very shallow portion of the plate boundary. However, it is still difficult to fully understand the in situ physical properties of the hanging wall of the plate boundary fault because of the limited logging data (gamma ray and resistivity) and limited cored intervals obtained during the drilling expedition. Local scale seismic images were previously obtained in a high-resolution seismic survey around the drill site (Chester et al. 2012, Nakamura et al. 2013), but a regional scale seismic section crossing the drill site had not been obtained. A regional scale seismic data is necessary to determine the velocity structure of the wedge and directly connect the drill site information to the background regional scale geological structure. To understand the structure and the physical properties of hanging wall sediments, a post-drilling multi-channel seismic (MCS) survey was conducted around the JFAST drill site. We processed the MCS data up to the pre-stack depth migration (PSDM) to produce an accurate depth seismic image and the P wave velocity structure. We also modeled travel-times of converted S wave arrivals observed at the ocean bottom seismographs (OBSs) to obtain the shear-wave velocity information around the drill site, which cannot be retrieved using the MCS data. We compare the seismic-derived velocity information with drilling results and controlled pressure V p and V s core measurements and discuss the similarities and differences between them.

Methods

Seismic survey KR13-01

The seismic survey cruise (KR13-01) was conducted in the Japan Trench region using R/V Kairei operated by Japan Agency for Marine-Earth Science and Technology (JAMSTEC) in January 2013. A tuned air gun array with 7,800 in.³ of total volume was fired every 50 m along the survey lines. A 444 channel streamer cable (approximately 6 km maximum offset) was towed to record the seismic signals with a sampling interval of 2 ms. The depth of the gun array and the streamer cable was 10 and 12 m, respectively. In this study, we use the data obtained along two seismic lines, JFD1 and JFS12, as shown in Figure 1.An OBS, developed for an operation deeper than 6,000 m, was deployed around site C0019 (Figure 1) to record the air gun signals with a sampling interval of 4 ms. The OBS JF1 was located at the lower most part of the Japan Trench landward slope, approximately 1 km north of the IODP site C0019 (Figure 1b). The OBS JF1 was not recovered by a normal self-popup recovery procedure, but it was recovered by the ROV KAIKO 7000II in April 2013 during the KR13-08 cruise.

Figure 1

The location map with seismic lines. (a) Regional scale bathymetry map of the Japan Trench region, off Miyagi, northeastern Japan. Red rectangle in the inset map corresponds to the area shown in Figure 1a. Yellow star denotes the epicenter of the Tohoku earthquake that occurred on 11 March 2011. Yellow lines indicate the seismic survey lines used in this study. Yellow numbers are the CDP numbers. Red inverted triangle is the location of the JFAST drill site C0019. (b) Close-up map around drill site C0019 with bathymetry contours. Green inverted triangle indicates the site location of OBS JF1. Blue lines show the seismic survey lines and blue numbers are the CDP numbers.

MCS data processing

The MCS data were first processed following a conventional procedure that includes minimum phase conversion, predictive deconvolution, common midpoint (CMP) sorting, velocity analysis, normal moveout, stacking, and post-stack time migration (PoSTM). Noise reduction by f-x projection (Soubaras 1995) and f-x prediction filtering (Canales 1984) was applied to reduce the swell noise and seismic waves by local earthquakes. Surface-related multiple elimination and parabolic radon transform were applied to suppress multiples. Pre-stack time migration (PSTM) analysis was applied to produce a fine-tuned time-domain seismic image. This PSTM section was used to establish the structural formation model for further PSDM analysis.

The MCS data of the line JFD1 were processed until PSDM to produce the depth seismic section and the corresponding P wave velocity model. A ‘layer-cake’ approach was used for PSDM velocity analysis where we first determined the velocity in the shallowest formation and then sequentially moved down to deeper formations. The velocity model v(z) in each formation has the following form: v(z) = v₀ + g (z - z₀), where z is the depth, v₀ is the P wave velocity at the top of the formation, z₀ is the top depth of the formation, and g is the velocity gradient. A depth section was created by PSDM with a defined layer-cake velocity model, and horizon semblance was examined to evaluate the velocity model. We determined v₀ and g to achieve the best improved horizon semblance over the target horizon by trial and error. Once a satisfactory layer-cake model was achieved, the velocity model was updated by a horizon-based residual velocity analysis which evaluates the moveout of migrated common reflection point (CRP) gathers using horizon semblance. The velocity was modified to shift the semblance peak to zero residual. The velocity model was finally updated by grid-based travel-time tomography to accommodate the local scale velocity variation. Clear but local reflective events (inter-layer segments) were picked for the input to the tomography, and grid-based velocity model was updated to flatten the CRP gathers at picked events. The velocity model cannot be resolved below the top of the oceanic crust due to the length of the streamer cable, so we use the deeper velocities determined in previous studies of the Japan Trench (Tsuru et al. 2000, Tsuru et al. 2002, Miura et al. 2005). Automatic gain control was used to enhance the deeper reflections in the gathers because we prioritized obtaining the best depth image and corresponding velocity model over amplitude preservation in this study.

OBS data analysis

The OBS recorded the seismic signal at longer offsets, and it is equipped with three component sensors (two horizontal and one vertical). As the number of the OBS used in this study was limited, the typical tomographic approach cannot be applied to the OBS data. Instead, we first applied the conventional tau-p/tau-sum method (Diebold and Stoffa, 1981, Shinohara et al. 1994) to obtain a 1D V p model. The envelope of the vertical component waveforms was used for the tau-p/tau-sum analysis to enhance the signal in the tau-p domain. Horizontal components of the OBS data record the shear wave arrivals which were originally emitted as P waves from the sounding source then converted to S waves before arriving at the OBS. In this study, we use the PPS-converted wave which was converted from P to S below the OBS location to estimate the average V p/V s in the layer/s between the seafloor and the conversion point (see Figure 2). The average V p/V s is calculated from following equation:

Figure 2

A schematic diagram showing a ray path of the P wave and PPS-converted wave. Information on parameters in Equation 1 is shown in this figure.

$$V\mathrm{p}/V\mathrm{s}~\left(2d\mathrm{t}+t_{\mathrm{c}}-t_{\mathrm{sf}}\right)/\left(t_{\mathrm{c}}-t_{\mathrm{sf}}\right)$$

(1)

where d t is the time lag between refracted P wave and the converted PPS wave, and t_c and t_sf are the two-way travel time of the conversion point and the seafloor shown on the time-domain seismic section.

P and S wave velocity measurements of the JFAST core sample

We measured the P wave and S wave velocities of sediment core samples obtained from the frontal prism during the JFAST drilling expedition. Six samples, retrieved between 690.4 and 818.5 mbsf (Table 1), were measured under controlled pore fluid pressure using laboratory instruments at Kochi University and the University of Wisconsin-Madison. The lithology of these cores was mudstone (Expedition 343/343T Scientists, 2013). The design of the experiment is similar to that employed in the previous studies on saturated marine sediments (e.g., Tobin et al. 1994, Hashimoto et al. 2010). The pore pressure was kept at 500 kPa for Core343-C0019E-7R (7R), and confining (effective) pressure was stepwise elevated from 1,000 to 18,000 kPa during the measurements. For other cores, velocity measurements were carried out while pressurizing and depressurizing. The pore pressure was kept at 1,000 kPa, and effective pressure was stepwise changed from 1,000 to 68,000 kPa and 68,000 to 500 kPa during the measurements. In this study, we used the velocities measured while pressurizing. For the measurements, the sample was formed into a cylindrical shape, approximately 3.8 cm for 7R and 2.45 cm for others in diameter, and 5.4 cm for 7R and 1 to 2 cm for other cores in length.

Table 1 List of the core samples used in this study

Results

Line JFD1 PSDM section

Pre-stack depth migrated section of the line JFD1 (Figure 3) clearly shows the characteristic structure of the Japan Trench subduction zone at the location of the JFAST drill site C0019. Seaward of the trench, pelagic and hemipelagic sediments with thickness of 300 to 500 m cover the oceanic basement reflections, and the Moho reflection is also imaged 5 to 6 km below the basement reflection. Both the sediments and the basement are offset by normal faults producing a horst and graben structure. In the vicinity of the trench axis, the structures imaged on the PSDM section are similar to those observed on high-resolution seismic profiles (Nakamura et al. 2013), e.g., imbricate structure in the trench axis graben (see also Figure 4). The drill site C0019 penetrates the wedge-shaped, seismically chaotic or transparent frontal prism imaged beneath the lowermost landward slope. The plate boundary at the drill site is located on a subducted horst block; the plate boundary reflection can be seen draping the horst at both seaward and landward edges. A few landward dipping weak reflections can be observed within the prism. These events are clearer than those on the high-resolution seismic profiles reported by Nakamura et al. (2013) because large volume air gun arrays and longer streamer cable were used to obtain the data for this study. Although these reflections are not really continuous and distinct, drilling results (e.g., Fulton et al. 2013, Ujiie et al. 2013) strongly suggest that Tohoku earthquake slip occurred along the plate boundary. The landward boundary of the frontal prism is a prominent landward dipping reflection corresponding to the backstop interface (Tsuru et al. 2000). The PSDM P wave velocity model (Figure 3c) shows a velocity inversion across the interface where backstop material overlies the frontal prism. The western part of the line JFD1, covering the upper to middle landward slope of the Japan Trench, shows a strong reflection 1,000 to 2,000 m below the seafloor which separates the slope sedimentary sequence from the deeper backstop unit, which was interpreted as Cretaceous sequences (e.g., von Huene and Culotta, 1989). Both the slope sediments and the underlying strong reflection are offset by normal faults (e.g., CDP 1300 to 1400). The vertical resolution of the seismic data can be estimated by the Rayleigh criterion of L/4, where L is the peak wavelength of the source at the local velocity of the medium, whereas the horizontal resolution is limited by the size of the first Fresnel zone; this is (L*d/2)^1/2, where d is the depth of the target. The horizontal resolution might be collapsed to L by the migration in the ideal case; however, it could be lower due to the noises and velocity errors used in the migration (e.g., Claerbout 1985, Stolt and Benson 1986, Yilmaz 2001). In this study, the typical vertical and horizontal resolution is estimated at approximately 15 to 20 m and 50 to 600 m in the incoming sediment and frontal prism, and 40 to 60 m and 150 to 1,000 m for the backstop interface, respectively.

Figure 3

Seismic sections and velocity model of line JFD1. The drill site location is indicated in this section. (a) The PSDM section without interpretation. (b) The PSDM section with interpretation. Interpreted formations are colored over the PSDM section shown in Figure 3a. (c) The PSDM interval velocity model overlain on the PSDM section.

Figure 4

Close- up view of the PSDM section of the line JFD1 around the frontal prism. Red dashed line is the backstop interface.

Velocity uncertainties in the PSDM analysis

We estimated the accuracy of the velocity derived from PSDM velocity modeling following Calahorrano et al. (2008), which evaluates the flatness of the CRP gathers at the target depth. A total of 13 velocity models with 5% step change (70% to 130% of original velocity model) in the velocities were tested. The results show that the velocity in the seaward part of the frontal prism around the JFAST site is determined with approximately 5% uncertainty, because the velocity models with 10% perturbation cannot flatten the CRP gathers in this area (Figure 5a). The velocity uncertainty is similarly estimated at approximately 5% in the incoming sediments seaward of the trench and at 5% to 10% in the Cretaceous sequences at its seaward edge (around CDP 6600). The uncertainty is larger at greater depth, for example, it increased to approximately 15% at the landward end of the frontal prism (CDP 6500 to 6700) (Figure 5b). In spite of the larger uncertainty in the landward part of the frontal prism beneath the backstop interface, the velocity inversion across the backstop interface mentioned above is still plausible, because the velocity above the interface (Cretaceous sequence) is 3.2 ± 0.3 km/s and that below (frontal prism) is 2.2 ± 0.3 km/s. In summary, the velocities shallower than approximately 10 km depth are generally well determined within 5% to 10% uncertainty, however, the velocities are poorly controlled so the depth image strongly depends on the reference velocity model in the area deeper than approximately 10 km below the sea level.

Figure 5

Examples of the velocity uncertainty estimation using CRP gathers. Each panel shows the CRP gather after PSDM using the velocity model with 5% step change (70% to 130% of original velocity model as shown above each gather). (a) CRP gather at CDP 8140. The target horizon is located at approximately 7,800 m in the CRP gather migrated with 100% velocity model. (b) CRP gather at CDP 6705. The target horizon is located at approximately 8,300 m in the CRP gather migrated with 100% velocity model.

Line JFS12 PoSTM section

Reflections from the seafloor and the subducting plate stratigraphy are recognized on the seismic profile of line JFS12 (Figure 6), but few internal reflections are observed in the frontal prism. The seafloor reflection is contaminated by artifacts, caused by sideswipes from adjacent slopes, whereas the subducting plate stratigraphy is clearly resolved at a relatively constant two-way travel time of 10,000 to 10,500 ms.

Figure 6

Post- stack time migrated section of the line JFS12. Projected location of the drill site C0019, and the OBS JF1 are indicated on this section.

OBS data

Figure 7a shows vertical component seismograms of air gun shots along the line JFS12 recorded at OBS JF1. The tau-p converted waveforms using the envelope of the same record, and the deduced 1D V p model are shown in the Figures 7b and 8, respectively. The V p in the sediment layer is between 1.9 and 2.2 km/s. Figure 9a,b shows the vertical and horizontal component recordings along the line JFS12 recorded at OBS JF1. Travel time was reduced by 6 km/s. On the vertical component (Figure 9a), a phase with an apparent velocity of approximately 6 km/s is clearly detected around 5.5 s intercept time. Horizontal component record (Figure 9b) also displays the phase with similar apparent velocity but different intercept time at around 7.1 s, which is interpreted as a P to S converted wave. PoSTM seismic section of JFS12 (Figure 6) exhibited strong reflections at the top of the chert layer, top of the oceanic crust and the Moho (approximately 12 s TWT not shown in Figure 6) below the seafloor so we consider that these are the most likely conversion points. This phase can be interpreted as the shear arrival which was converted from P to S around the sediment/oceanic-crust boundary below the OBS location because it has an apparent velocity similar to the typical V p value at the top of the oceanic crust (approximately 6 km/s). We can calculate average V p/V s in the sediment beneath the OBS JF1 using Equation 1, where d t (time lag), t_c (two-way time of conversion point below the OBS), and t_sf (two-way time of seafloor at OBS location) is 1.6 ± 0.1, 10.05 ± 0.05, and 9.12 ± 0.05, respectively. The uncertainty was evaluated with possible reading errors for each phase which depends on the wavelength of the phase. V p/V s is 4.4 + 0.7/-0.5 assuming the conversion point at top of the oceanic crust. An alternative conversion point could be the top of the chert layer, which is approximately 100 ms shallower than the top of the oceanic crust beneath the OBS location. If we assume the P to S conversion at this boundary, the V p/V s is 4.9 + 0.8/-0.7. Other possible conversion points could be the boundary between oceanic layer two and three and the Moho discontinuity. However, the apparent velocity of this PPS phase is approximately 6 km/s. This observation suggests that this phase propagated in the oceanic layer two not in layer three, because V p in oceanic layer three is generally higher than 6.5 km/s, as can be observed in the survey line 15 km north of the OBS JF1 (Miura et al. 2005), and the velocity in the upper most mantle is 7.7 km/s in the same line (Miura et al. 2005). These velocities are clearly higher than the apparent velocity of this PPS-converted phase. We modeled the travel-times of the observed phases discussed above with a velocity structure with high V p/V s (4.2 in this case) in the sediment layer (Figure 9c). The observed phases with approximately 6 km/s of apparent velocity are well explained as the P wave traveling through oceanic crust layer 2, and PPS-converted wave converted at the sediment/crust boundary beneath the OBS location (see also Figure 9a,b). In summary, the average V p/V s in the hanging wall sediment should be larger than 3.9 around the JFAST drill site.

Figure 7

OBS data and its tau- p conversion. (a) The vertical component seismograms at OBS JF1 from shots along the line JFS12. The data were band-pass filtered (3 to 12 Hz). Some major phases are indicated in this section. (b) The same seismograms as Figure 7a but in tau-p domain. The envelope of the seismograms in Figure 7a was converted into tau-p domain. Major phases are indicated in the section.

Figure 8

P wave velocity model and measurements around the JFAST site. Red and green lines indicate the velocity models derived from PSDM analysis (CDP 8225) and OBS data analysis (JF1), respectively. Blue line is the averaged interval velocity estimated from the drilling (Expedition 343/343T scientists 2013). Cyan solid circle denotes the P wave velocity measured from the core samples under the controlled effective pressure. The velocity is estimated from the core experiments (Figure 10) at an in situ effective pressure calculated from the density profile, which was computed from the resistivity logging data (Expedition 343/343T scientists 2013). Note that the OBS location is 1 km north (see Figure 1b), and the water depth is deeper than the site C0019.

Figure 9

The vertical and horizontal component OBS data and velocity model for travel time modeling. (a) The vertical component seismograms at OBS JF1 with the travel time reduced with 6 km/s. Green arrows indicate P wave arrivals that propagated through the upper oceanic crust, and green dots are the modeled travel time of this P wave calculated from the velocity structure shown in Figure 9c. (b) Same as Figure 9a but for a horizontal component. Black arrows indicate the S wave arrival with apparent velocity of approximately 6 km/s, which is interpreted as the PPS-converted wave beneath the OBS location. Black dots are the modeled travel time of this PPS phase calculated from the velocity structure shown in Figure 9c. (c) Ray paths and four-layered velocity structure to model the travel time of P wave arrival and converted S wave arrival shown in Figure 9a,b. Black inverted triangle is the OBS location. Blue lines are the structure boundaries. P wave velocity values are indicated to the right of this figure. V p/V s is 1.7 in the crustal layer and 4.2 in the sediment layer. Green and black thin lines are the ray paths for P wave propagating upper oceanic crust and PPS-converted wave which was P-to-S converted beneath the OBS location.

Velocities measured from core samples

Figure 10 shows the velocity changes with effective pressure obtained from the core sample experiments. V p and V s approximately ranging from 1.84 to 3.29 km/s and from 0.80 to 1.16 km/s, respectively, over the applied effective pressure range. V p/V s vary between 1.94 and 3.16, corresponding to Poisson's ratio values of 0.32 to 0.44. V p, V s, and V p/V s values at in situ condition at each coring depth were estimated assuming hydrostatic conditions (Figure 8, Table 2). The lithostatic pressure was estimated from a density curve that was in turn calculated from resistivity logging data, assuming a constant grain density of 2.50 g/cm³ (Expedition 343/343T Scientists, 2013). The range of estimated values for in situ V p, V s, and V p/V s are 2.00 to 2.48 km/s, 0.88 to 1.10 km/s, 2.05 to 2.48, respectively.

Figure 10

Velocity measurements of the core samples under controlled effective pressure. (a) P wave and (b) S wave. Dark red, red, orange, magenta, green, blue lines, and symbols indicate the measured velocities for Core 4R, 6R, 7R, 8R, 15R, and 16R, respectively.

Table 2 In situ velocities, V p/V s, and Poisson's ratio estimated from core experiments

Discussions

Seismic structure and velocity in the frontal prism

The frontal prism is located at the seaward edge of the hanging wall, and it is thought to have been horizontally displaced more than 50 m during the Tohoku earthquake (Fujiwara et al. 2011, Ito et al. 2011). Our PSDM image (Figures 3a and 4) shows a relatively transparent frontal prism, although several landward dipping discontinuous reflections can be distinguished (Figure 4). Some of these reflections extend from the plate boundary to the seafloor and have been previously interpreted as reverse faults (e.g., Tsuji et al. 2013); however, the lack of stratigraphy in the frontal prism makes it difficult to determine the sense of slip. The seismic velocity within the frontal prism is approximately 2.0 km/s in average and 2.5 km/s at maximum (Figure 3c). The velocity model is comparable with the model in Tsuru et al. (2000) obtained in the Japan Trench approximately 50 km north of our survey area, but the model in this study has slower velocity in the landward deeper part within the frontal prism. The difference is probably a consequence of the lower velocity gradient value in the velocity model adopted in this study. Park et al. (2010) obtained a detailed seismic image and velocity volume from a 3D reflection seismic data in the Nankai subduction margin off the southwest Japan. Their velocity model shows that the P wave velocity in the hanging wall accretionary prism is approximately 2.0 km/s at the trough axis, but it increases to approximately 3.0 km/s at 10 km landward of the trough axis. They reported the presence of a low velocity zone (LVZ) within the outer wedge of the accretionary prism, 10 to 25 km landward of the trough axis; however, the velocity is 2.7 to 3.2 km/s in the LVZ.

P wave velocities around the site C0019

We obtained V p around the drill site C0019 from two different seismic data analyses: one is from the PSDM analysis using the MCS data and the other is the 1D velocity derived from tau-p/tau-sum analysis on the OBS data (Figure 8). The PSDM velocity has lower velocity (1.6 km/s) at the top of the sediment layer and higher velocity (2.3 km/s) at the bottom, with larger gradient than the OBS velocity. Small scale velocity change within the frontal prism is not well resolved from the PSDM analysis due to the lack of internal reflections (Figures 4 and 5). However, the averaged value of the PSDM velocity in the frontal prism formation is approximately 2.0 km/s, which is comparable with that obtained from the OBS data analysis (Figure 8). The comparison of the seismic data with the drilling results during the Expedition 343 indicated that averaged interval velocity of the interval between the seafloor and the strong reflection near the top of the chert layer is approximately 1.9 km/s which is also comparable to the OBS velocity and the averaged PSDM velocity (Figure 8). Estimated in situ V p values are 2.00 to 2.23 km/s for cores 4R, 6R, 7R, and 8R, which is also consistent with the velocity obtained from the seismic data analysis (Figure 8). For deeper cores, 15R and 16R, in situ V p is slightly higher, ranging between 2.35 to 2.48 km/s. These values match with the PSDM velocities (Figure 8); however, the PSDM velocity curve in this depth range (7,700 to 7,800 mbsl) could be affected by the vertical smoothing during the velocity model building. The higher velocity values measured from core samples may represent the faster velocity layer at the bottom of the prism, which is below the nominal resolution of the seismic system at this depth level.

High average V p/V s in the frontal prism

According to our analysis, the average V p/V s ratio in the prism around the site C0019 (or OBS JF1) is 4.4 + 0.7/-0.5 or larger. This is equivalent to a Poisson's ratio > 0.46 and V s < 0.48 km/s. V p and V s under the saturated and confined pressure situation (Figure 10, Table 2) give much lower V p/V s 2 to 2.5.

We have compared our results with existing empirical V p-V s relationships. We have used mudrock line for clastic silicate rock (Castagna et al. 1985), which is often used to evaluate the V p and V s in marine sediments. Following the mudrock line V p = 1.16 V s + 1.36, the V p/V s can take significantly large value if the V p is low. The V p/V s is estimated at 4.08 assuming V p = 1.9 km/s (5% reduction from 2.0 km/s), which is located at the lowest possible range from our observation if we consider all uncertainties on the velocity analysis to reduce V p/V s. We note that the core measurements were limited to the section deeper than 600 mbsf (Chester et al. 2012), and that the velocity measurements can only be carried on the samples with enough stiffness. It is likely that the shallower frontal prism, which was not sampled during the Expedition 343, and/or the intervals with poor recovery that did not provide adequate samples for measurement, could have larger V p/V s increasing the average V p/V s value in the hanging wall sediments. Large V p/V s values have been reported in the sediments on the incoming plates seaward of the trench and trench fill sediments. The V p/V s of the incoming sediments on the Pacific plate in the Kuril Trench was estimated to be approximately 8 from the PPS-converted wave observed by the OBSs (Fujie et al. 2013). Peacock et al. (2010) reported high Poisson's ratio (>0.45) in the trench fill sediments in the Nankai Trough, which corresponds to the V p/V s values larger than 3.3. Similar high V p/V s ratio (approximately 3) was reported for the incoming sediments in the Nankai Trough (Tsuji et al. 2011). On the other hand, Tsuji et al. (2011) reported that the V p/V s value is approximately 2 at the toe of the hanging wall accretionary prism landward of the trough axis in the Nankai Trough, which is approximately half of our observation in the Japan Trench. The Poisson's ratio of sediments is affected by the consolidation, i.e., unconsolidated sediments show high Poisson's ratio (e.g., Prasad 2002). Unconsolidated sediments in the shallowest portion of the prism could contribute to increase the average V p/V s and Poisson's ratio. Tsuji et al. (2011) pointed out that the sand-rich turbidite could reduce the V p/V s (and Poisson's ratio). In the Japan Trench, at least at the site C0019, sand-rich sediment is not observed in core samples and not suggested by gamma-ray log data. The lack of the sand-rich sediments might be one of the possible reasons to cause the high Poisson's ratio in the Japan Trench prism toe.

Conclusions

A newly conducted seismic experiment around the JFAST drill site provides a regional-scale depth seismic image and the corresponding velocity models. The obtained PSDM profile exhibits seismically transparent or chaotic frontal prism with several semi-continuous landward dipping reflections beneath the toe of the Japan Trench landward slope. The P wave velocity model derived from the PSDM analysis shows that frontal prism has the low average interval velocity approximately 2.0 km/s. The backstop interface is clearly imaged, and there is a velocity inversion from the Cretaceous sequences to the underlying frontal prism. The velocity values around the drill site derived from the PSDM analysis are reasonably comparable with the 1D P wave velocity model estimated from OBS data. The controlled effective pressure core P wave velocity is also similar to the velocities from the seismic data analysis. The averaged V p/V s calculated from the analysis of seismic data is approximately 4.4 in the hanging wall sediments around the drill site from OBS data, which is considerably larger than that calculated from core measurements. To reconcile these two apparently contradictory observations, it is necessary that the shallower part of the hanging wall sediments, which were not retrieved from core measurements, should have very high V p/V s values. The OBS-derived V p/V s in the hanging wall sediments is also significantly higher than that in the toe of other subduction zones.