| Citation: | Shengquan Tang, Xueen Chen, Zhi Zeng, Xin Liu. Numerical investigation of the South China Sea deep circulation[J]. Acta Oceanologica Sinica, 2022, 41(5): 1-11. doi: 10.1007/s13131-021-1879-y
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The Izu-Bonin-Marina arc (IBM) subduction system is a typical representative of the large-scale convergence boundary in the world, having strong lithospheric deformation and magmatic activity in the West Pacific. It forms a typical “trench-arc-basin” system with an eastward transition of the back-arc spreading due to the westward subducting Pacific Plate (Fig. 1). It is widely considered as an ideal area to study the “subduction factory” as well as the seismic activities of the subduction zone (Ishizuka et al., 2011a, b). In the western part, the IBM subduction system has a remnant arc, namely the Kyushu-Palau Ridge (KPR); whereas the modern IBM volcanic island arc belt (such as the Izu-Ogasawara Ridges and Mali Yana Island Arc) lies in the east. Several Cenozoic oceanic basins developed in-between, including the Shikoku Basin, Parece Vela Basin (PVB), Ogasawara Trough, and Mariana Trough (Fig. 1).
The KPR extends from the Nankai Trough in the north to the northern part of the Palau Archipelago in the south. It is a bathymetric high extending through the Philippine Sea Plate with a total length of 2 600 km (Fig. 1). It was once connected with the modern IBM island arc belt before the splitting of the proto-IBM arc and the back-arc spreading with the continuous retreat of the Pacific Plate subduction at about 30 Ma BP (Stern et al., 2004). Therefore, the KPR should be firstly built by the initial subduction between the proto-Pacific Plate under the West Philippine Basin (WPB), and then modified by the magmatic activity after the breakup of the proto-IBM island arc. However, how magmatism controlled the growth of the KPR is still debatable.
Seismic velocity models can be used to provide a crisis information for the mechanisms of the growth of the island arc crust. The previous deep reflection/refraction seismic explorations carried out on the KPR were completed mainly by Japanese scientists (Murauchi et al., 1968; Arisaka et al., 2003; Nishizawa et al., 2007, 2016). Especially during 2004–2008, the Japan Agency for Marine-Earth Science and Technology conducted a series of seismic experiments on the KPR and presented 27 wide-angle seismic profiles to understand its lithospheric structural changes from north (31°N) to south (13°N) (Nishizawa et al., 2016). Their results showed that the KPR has a large variation in crustal thickness (8–23 km), which is generally larger than those oceanic crust of the surrounding back-arc basin, such as the PVB in the east and the WPB in the west. The growth of the thick crust is accommodated mainly by accretion of the lower crust (6.8–7.0 km/s), whereas for crustal thickness greater than 20 km, it also has a relatively thick (>5 km) middle crust with a P-wave velocity (
According to the above, seismic experiments focused mainly on the northern part of the KPR (north of 15°N) (Fig. 1), and the crustal structure of the southern part (south of 15°N) has limited data and is less understood. To better understand the crustal structure of the southern KPR, this study used a 217 km long wide-angle seismic profile (ID: KPR2020-2) to estimate the structure of the crust and the uppermost mantle across the KPR near 12°N. Comparing it with the crustal structure of the above two profiles will provide key information on the growth of the KPR in this area.
Based on petrological and geomagnetic data, the tectonic evolution history of the Philippine Sea Plate has been well understood (Stern and Bloomer, 1992; Bloomer et al., 1995; Kobayashi et al., 1995; Okino et al., 1999; Hall, 2002; Stern et al., 2004). The first stage is the formation of the WPB, which is a back-arc basin developed with the seafloor spreading starting at around 55 Ma BP (Deschamps and Lallemand, 2002). Then, during 50–52 Ma BP, the Paleo-Pacific Plate began to subduct beneath the WPB, forming initial lithosphere subsidence along the eastern edge of the WPB (Ishizuka et al., 2011a). At 43 Ma BP, when the abrupt change of the Pacific Plate movement from NNW to NWW occurred, the subsidence of the lithosphere evolved into subduction (Richards and Lithgow-Bertelloni, 1996), indicating that the initial subduction lasted about 7 Ma (Ishizuka et al., 2011a). The International Ocean Discovery Program (IODP) has successively carried out two expeditions in this area (IODP Expeditions 351 and 352). Their results indicated that the fore-arc seafloor spreading occurred before the initiation of the subduction, then with the continuous subduction of the proto-Pacific Plate, the proto-IBM arc was formed within the fore-arc oceanic basin (Arculus et al., 2015; Reagan et al., 2017; Ishizuka et al., 2018). Based on the age and geochemical characteristics of the dredged samples along the entire KPR, Ishizuka et al. (2011b) concluded that the activity timing of KPR is 25–48 Ma BP, but most ages of the dredged samples fall into a narrow range of 25–28 Ma BP. The proto-IBM arc is dominated by island arc porphyry and calc-alkaline basalt (Ishizuka et al., 2018). After the formation of the proto-IBM arc, rifting and seafloor spreading occurred in the proto-IBM arc at about 30 Ma BP, forming the Shikoku Sea Basin (30–15 Ma BP; Okino et al., 1994) and the PVB (29–12 Ma BP; Okino et al., 1999) between the residual KPR and the present IBM arc (Fig. 1). These two spreading systems connected at 20 Ma BP and ceased spreading around 15 Ma BP. The spreading center jumped eastward with the retreat of the Pacific Plate, which opened the Mariana Trough at 3–4 Ma BP (Stern et al., 2004).
The seismic source was a 4×32.7 L air-gun array shot at an average shooting interval of 200 m with a pressure of 10.79 MPa every 78–97 s. Here, this study focuses on the 217 km seismic profile KPR2020-2 with 1 083 shots (red line in Fig. 2). The OBS is composed of 4.5 Hz four-component geophones. Ten OBSs recorded good data sets, whereas OBS1 and OBS2 in the west and OBS13 in the east failed (Fig. 2). This study determined P wave velocities using the hydrophone component. For OBS5, the vertical component was used, as poor signals were recorded in its hydrophone component. The processing of OBS data included correction for OBS clock drift, relocation of OBSs and shots using direct arrivals, and bandpass filtering at 4–20 Hz. A final straight-line approximation of the profile was determined by least squares fit to all the shots on the profile. The depth of each OBS was first roughly determined from multi-beam bathymetric data, and then refined by fitting direct arrivals.
In general, the seismic data quality is good. Phases are identified using initial travel time modeling. This study identified the direct water wave labeled Pw, the refracted wave from oceanic Layer 2 labeled P2, the refracted wave from oceanic Layer 3 labeled P3, the Moho reflection labeled PmP, and the refracted wave from the upper mantle labeled Pn.
Clear Pw, P2, P3, PmP and Pn phases were observed at most OBSs, especially OBSs5–11 deployed above the KPR (Figs 3–7). A maximum offset of the Pn phase was observed up to 85 km, which made a good overlap control for the model. Travel-time uncertainties were dominated by picking uncertainties, which were estimated as 50 ms, 60 ms, 80 ms, 100 ms and 120 ms for Pw, P2, P3, PmP and Pn arrivals, respectively.
OBS7 was deployed at the western part of the KPR. Clearly, P2, P3, PmP and Pn phases were observed at both sides of OBS7, PmP phase was found at offsets about 20 km and 40 km of its western and eastern sides, respectively (Fig. 3). OBS8 was deployed 15 km east of OBS7. Clearly, P2, P3, PmP and Pn phases were found at its both sides, and PmP phase was found at offsets starting at 20 km and 33 km of its western and eastern sides, respectively (Fig. 4). OBS9 was deployed at the center of the KPR, 15 km east of OBS8, and P2, P3, and Pn phases were also found at both its sides, but PmP phase was found only at offsets starting at 35 km of its eastern side (Fig. 5). OBS10 was deployed at 15 km east of OBS9. Clearly, PmP phase was observed at offsets of 30 km and 15 km at its western and eastern sides, respectively (Fig. 6). Although PmP phase was found only at the western side of OBS11 with an offset starting at about 30 km (Fig. 7), P2, P3, and Pn phases were observed clearly at OBS10 and OBS11. A few arrivals may not be fitted well, which may be due to the rugged topography across the KPR.
Travel time modelling and inversion approach of Zelt and Smith (1992) were used to construct velocity models. The initial model consisted of two crustal layers, representing oceanic layers 2 and 3, with linear gradients within these layers and no velocity discontinuity between them. Oceanic Layer 2 was 2 km thick and had velocities of 1.8 km/s at the top and 6.4 km/s at the bottom, whereas oceanic Layer 3 was 4 km thick and had velocities of 6.4 km/s at the top and 7.0 km/s at the bottom. The upper mantle had a velocity of 8.0 km/s at the top. The horizontal node spacings within oceanic Layers 2 and 3 were 5 km. In the upper mantle, the node spacing was 50 km. This model was based on global averages of the oceanic crustal structure (Kennett, 1982; White et al., 1992). As described by Zelt and Smith (1992), velocities and boundaries were initially adjusted manually by trial and error. After this forward modeling, a damped least squares inversion was conducted to optimize the velocity within each layer, while keeping the layer boundaries fixed.
Along the profile KPR2020-2, the average thicknesses of oceanic crust Layer 2 and oceanic crust Layer 3 were ~3.5 km and 4.7 km, respectively, and the average velocities in Layer 2 and Layer 3 were 4.2 km/s and 6.7 km/s, respectively. As a result, the vertical velocity gradient within Layer 2 was high (average is 1.2 s−1), while within Layer 3 was low (average is 0.2 s−1). The velocity at the top of the upper mantle was 7.8 km/s. According to the tomography features and internal structures, this study divided the seismic profile into three parts: WPB (0–70 km), KPR (70–170 km), PVB (170–217 km).
Beneath the WPB, Layers 2 and 3 had roughly constant thickness (2.7 km and 3.8 km, respectively), and different vertical velocity gradients (~1.6 s−1 and ~0.2 s−1, respectively). In general, lower crustal velocity of 7.0 km/s was observed at the eastern margin (60–70 km) of the WPB with few high-velocity lower crustal layers (7.3 km/s) (Fig. 8a). The Moho lies at ~12.2 km below sea level, resulting in a crustal thickness of 6.5 km. Part of the Moho reflector was controlled well by PmP (Fig. 8a).
Beneath the major part of the KPR, both crustal thickness and velocity show lateral heterogeneous. Thickness of Layer 2 changed little (between 3.7 km and 4.2 km), although the seafloor depth changed a lot (from 2.5 km to 5.0 km). The thickness of Layer 3 varied from 4.0 km at the edges of the KPR to 6.7 km in the center. Velocity varied at the top of Layer 2 (seafloor, from 1.6 km/s to 3.2 km/s) and at the bottom of Layer 3 (6.7 km/s to 7.2 km/s), and the velocity between Layers 2 and 3 showed no discontinuities at 6.1 km/s, which is lower than that beneath the WPB and PVB (6.4 km/s). The depth of the Moho reflector was well controlled by PmP (Fig. 8a), which varied from 12.7 km to 14.0 km below sea level, sketching a relatively thicker crust ranging from to 8.2 km to 11.3 km.
The crustal structure beneath the PVB was found to be similar to that of the WPB, both Layers 2 and 3 have roughly constant thickness (3.0 km and 4.4 km, respectively), but different vertical velocity gradients (~1.5 s−1 and ~0.2 s−1, respectively). The average
Pick uncertainties and the travel-time misfit of the best model are provided in Table 1. The overall root-mean-square (RMS) misfit was 113 ms, and the misfit increased slightly with depth and offset. The overall χ2 value was 1.443, with 95.0% of picks fitted, and the normalized travel time misfit suggested that the model was suitably parameterized, with a travel-time misfit a slightly bigger than the pick uncertainty. The numbers of rays through each cell were generally larger than 10 and reached over 100 (Fig. 8b), indicating that the model was well constrained. By using a perturbation test (Zelt and Smith, 1992; Muller et al., 1997), the uncertainty of the Moho depth was found to be ±0.3 km.
| Phase | Total picks | Inverted picks | Fit ratio/% | RMS/ms | $\ \chi^2$ |
| Pw | 456 | 447 | 98.0 | 36 | 0.521 |
| P2 | 604 | 543 | 89.9 | 101 | 2.813 |
| P3 | 2 100 | 1 929 | 91.9 | 98 | 1.528 |
| PmP | 1 069 | 1 053 | 98.5 | 90 | 0.913 |
| Pn | 2 126 | 2 124 | 99.9 | 146 | 1.476 |
| All | 6 416 | 6 094 | 95.0 | 113 | 1.443 |
| Note: RMS, root-mean-square. | |||||
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Two-dimension (2D) gravity modeling and isostatic analysis can give further constraints on the crustal model. The forward gravity response of the 2D gravity modeling is based on the 2D algorithm by Talwani et al. (1959). The free-air gravity anomaly is derived from Sandwell et al. (2014), which is a global 1′ × 1′ gravity grid. The crustal and upper mantle density model was made from the P wave velocity model in this study, where the densities for each polygon were derived from RAYINVR using its internal velocity to density conversion (Zelt and Smith, 1992). The result showed a reasonable agreement between the calculated and observed gravity anomalies along the WPB and PVB, whereas the calculated gravity under the KPR was higher than the observed (20–40 mGal, 1 Gal=1 cm/s2) (Fig. 9). This difference might be due to the low resolution of the long-wavelength satellite derived gravity anomalies. However, the overall trend of the calculated gravity filed fits well with the observed trend, which makes good constraints on the crustal structure of the seismic refraction profile.
For isostatic analysis, this study calculated the pressure based on the crustal and upper mantle density model down to depth of 20 km (Fig. 9). The pressures along the WPB and PVB were 0.485 GPa and 0.495 GPa, respectively. There was no regional trend along both WPB and PVB. The difference between these two is probably due to the different oceanic lithospheric densities caused by the different ages of oceanic crust there. The pressure under the ridge was 0.51–0.52 GPa, 5.1% higher, suggesting that the KPR grew on oceanic lithosphere with some flexural strength.
Early studies have shown that the velocity structure of the mature intra-oceanic island arc crust is quite different from that of submarine volcanoes that grow on the oceanic crust. The main difference is that the island arc has a thicker middle crust larger than 5 km (6.0–6.5 km/s) (Holbrook et al., 1999; Takahashi et al., 2008). The growth of the island arc results mainly from the accretion of both the middle and lower crust. The first stage includes the successive basaltic underplating caused by the partial melting of the underneath subduction plate. The second stage involves the formation of the middle crust, which comes from the initial basaltic crust differentiating to generate a crust with intermediate to felsic components with higher SiO2 content (Takahashi et al., 2007, 2008).
Previous studies show that the development of the southern KPR has two stages (Stern et al., 2004). The first stage includes early initial island arc formation caused by the subduction of the paleo-Pacific Plate under the WPB starting at 45 Ma BP (Ishizuka et al., 2011a), forming the proto-IBM arc. The second stage involves the splitting of the proto-IBM arc and back-arc seafloor spreading of the PVB between 30–28 Ma BP (Stern et al., 2004; Okino et al., 1994; Ishizuka et al., 2011a; Grevemeyer et al., 2021), producing the relic KPR and the present IBM island arc. If the KPR is composed of the initial island arc, the crustal structure should resemble a velocity structure of the mature arc island. However, if the growth of the KPR is dominated by the magmatism related to the later stage back-arc spreading, the original velocity structure of the KPR could be modified, which could be similar to the structure of typical oceanic submarine volcanoes.
Based on the seismic velocity model, the KPR crust of this study can be divided into the upper crust (<6.4 m/s), and lower crust (6.4–7.2 km/s). The crustal thickness of the KPR is up to 12 km, but it gradually decreases to 5–6 km on both sides adjoining the WPB and PVB. The crustal structures of the WPB and PVB are consistent with results obtained from earlier seismic studies in this area (Arisaka et al., 2003; Nishizawa et al., 2007, 2016). The crustal velocity structure under the KPR is comparable to the profile Kpr41, but shows remarkable difference with that of the profile Kpr40. The latter has a thick (>5 km) middle crustal layer with a thick (~5 km) high-velocity lower crustal layer of 7.2 km/s. (Nishizawa et al., 2016) (Fig. 2). Compared to the Atlantic Ocean 0–127 Ma oceanic crustal structures, the velocity structure under the KPR is similar to that of the oceanic crust (White et al., 1992) (Fig. 10). The thick middle crust (>5 km) that observed in the mature intra-oceanic island arc crust was not observed in the velocity model of this study, which indicates that the KPR in the study area has immature island arc nature.
Back-arc spreading usually accompanies arc development (Martinez and Taylor, 2002; Dunn and Martinez, 2011). Consequently, magmatism during the arc splitting process could be controlled by pressure-release partial melting of fertile mantle. The crustal structure formed by this process is similar to the velocity structure of normal oceanic crust.
The subducting slabs could also generate arc magmatism affecting KPR crustal accretion during the breakup of the arc island. In this case, it will form a thick high-velocity lower crustal layer (7.2–7.6 km/s) along the western margin of the PVB, which mainly has mafic-to-ultramafic crustal composition underplated the lower crustal layer (Eason and Dunn, 2015). However, the seismic velocity structure shows that the average
The main formation stage of the KPR can be estimated by the plate strength at the time of the KPR loading. The IODP results show that the initial stage of the KPR formation is built by the arc magmatism (~45 Ma BP), which grew on the oceanic basin created by the fore-arc seafloor spreading starting at 50–52 Ma BP (Arculus et al., 2015; Reagan et al., 2017; Ishizuka et al., 2018). If most of the crust accretion of the KPR comes from this process, then the KPR should be formed on an oceanic plate (oceanic age 5–7 Ma) with low lithospheric plate strength. In this case, the crust should have a mountain root with nearly local isostasy compensation. At around 30 Ma BP, the rejuvenate of the KPR grew on an oceanic plate with age older than 20 Ma. If that so, the crustal structure should have some regional compensation as the ridge grew on an oceanic plate with some flexural strength. The crustal model of this study showed that the pressure under the KPR was 0.51–0.52 GPa, which is 5.1% higher than the adjacent PVB and WPB. This implies that there is some regional compensation during the loading of the KPR. Thus, this study exclude the effects of initial arc magmatism during the formation of the KPR.
In conclusion, the seismic crustal velocity structure shows that the velocity structure of KPR is more similar to an oceanic crust rather than a mature island arc. The estimation of the plate strength during the KPR loading suggests that the KPR is built mainly by the magmatism during the rifting of the proto-IBM arc between 30–28 Ma BP. The absence of the middle crust layer, larger than 5 km (6.0–6.5 km/s) and high velocity lower crustal layers (7.2–7.6 km/s) indicate that the arc magmatism plays a less important role in the KPR formation.
Travel-time modeling of active-source wide-angle seismic P wave data from OBSs deployed crossing the WPB, KPR, and PVB led to the following conclusions:
(1) This study show a high resolution crustal
(2) 1 D velocity tests show that the seismic velocity structure of the KPR is comparable to the Atlantic oceanic crust (0–127 Ma), which implies a typical oceanic crust beneath the KPR. Isostatic analysis shows that there is some regional compensation during the loading of the KPR, indicating that the initial arc-magmatism is not the dominant process of the KPR formation. The absence of the thick middle crust (6.0–6.5 km/s) and thick high-velocity lower crust layer (7.2–7.6 km/s) suggest that arc-magmatism plays a less important role in the formation of the KPR.
We thank the crew of the R/V Dayanghao, and the technical staff and researchers involved in the West Philippine Sea 2020 Survey.
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| 1. | Panfeng Li, Xuwen Qin, Yong Zhang, et al. Along-Strike Morphologic Variations of the Kyushu-Palau Ridge at 13°–17° N and Their Tectonic Implications. Russian Journal of Pacific Geology, 2024, 18(2): 220. doi:10.1134/S1819714024020052 | |
| 2. | Xiaodong Wei, Weiwei Ding, Aiguo Ruan, et al. Crustal structure of the central and southern Kyushu-Palau Ridge: Implications for intra-oceanic arc evolution. Journal of Asian Earth Sciences, 2024, 267: 106151. doi:10.1016/j.jseaes.2024.106151 | |
| 3. | Jie Zhang, Jiabiao Li, Weiwei Ding, et al. Crustal structure and magmatism of the southern Kyushu-Palau ridge. Tectonophysics, 2023, 858: 229862. doi:10.1016/j.tecto.2023.229862 |
Figures(10) / Tables(1)
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Xiongwei Niu, Pingchuan Tan, Weiwei Ding, Wei Wang, Yao Wei, Xiaodong Wei, Aiguo Ruan, Jie Zhang, Chunyang Wang, Yong Tang, Jiabiao Li. Oceanic crustal structure and tectonic origin of the southern Kyushu-Palau Ridge in the Philippine Sea[J]. Acta Oceanologica Sinica, 2022, 41(1): 39-49. doi: 10.1007/s13131-021-1978-9
| Phase | Total picks | Inverted picks | Fit ratio/% | RMS/ms | $\ \chi^2$ |
| Pw | 456 | 447 | 98.0 | 36 | 0.521 |
| P2 | 604 | 543 | 89.9 | 101 | 2.813 |
| P3 | 2 100 | 1 929 | 91.9 | 98 | 1.528 |
| PmP | 1 069 | 1 053 | 98.5 | 90 | 0.913 |
| Pn | 2 126 | 2 124 | 99.9 | 146 | 1.476 |
| All | 6 416 | 6 094 | 95.0 | 113 | 1.443 |
| Note: RMS, root-mean-square. | |||||
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