2018
DOI: 10.1029/2018gl077436
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Radial and Azimuthal Anisotropy Tomography of the NE Japan Subduction Zone: Implications for the Pacific Slab and Mantle Wedge Dynamics

Abstract: We investigate slab and mantle structure of the NE Japan subduction zone from P wave azimuthal and radial anisotropy using travel time tomography. Trench normal E-W-trending azimuthal anisotropy (AA) and radial anisotropy (RA) with VP V > VP H are found in the mantle wedge, which supports the existence of small-scale convection in the mantle wedge with flow-induced LPO of mantle minerals. In the subducting Pacific slab, trench parallel N-S-trending AA and RA with VP H > VP V are obtained. Considering the effec… Show more

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Cited by 14 publications
(15 citation statements)
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References 28 publications
(42 reference statements)
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“…The convergence of the ILM and ELM has caused eastward asthenospheric flow (Yin & Taylor, 2011), which may induce the E‐W trending SWB features. Since the deformation pattern in the mantle wedge is almost horizontal if there is no small‐scale convection (Ishise et al., 2018), a positive RAN should be observed, which is different from our results. Therefore, we suggest that small‐scale convection occurs above the ILM (L1 and H1’ in Figures 3 and 4).…”
Section: Discussioncontrasting
confidence: 99%
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“…The convergence of the ILM and ELM has caused eastward asthenospheric flow (Yin & Taylor, 2011), which may induce the E‐W trending SWB features. Since the deformation pattern in the mantle wedge is almost horizontal if there is no small‐scale convection (Ishise et al., 2018), a positive RAN should be observed, which is different from our results. Therefore, we suggest that small‐scale convection occurs above the ILM (L1 and H1’ in Figures 3 and 4).…”
Section: Discussioncontrasting
confidence: 99%
“…On the basis of the above discussions, the LVZ above the ILM can be considered as a “mantle wedge” (L1 in Figure 4a). Results of both numerical simulation and RAN tomography have illustrated the small‐scale convection occurring in the mantle wedge (Ishise et al., 2018; Liu & Zhao, 2017), in which the fast polarization directions in the forearc inferred from SWB measurements are perpendicular to the subduction direction (Huang et al., 2011), and negative RAN prevails in the mantle wedge (Liu & Zhao, 2017). The convergence of the ILM and ELM has caused eastward asthenospheric flow (Yin & Taylor, 2011), which may induce the E‐W trending SWB features.…”
Section: Discussionmentioning
confidence: 99%
“…On the other hand, Ishise et al (2018) also conduct a P-wave radial anisotropy study of NE Japan and find negative radial anisotropy (V PH < V PV ) in the mantle wedge and positive radial anisotropy (V PH > V PV ) in the subducting slab. Instead of invoking different olivine types, Ishise et al (2018) explain their results by small-scale convection in the mantle wedge assuming an A-type olivine fabric. Numerical simulations by Morishige and Honda (2011) indicated steep downflows and gentle upflows, which would produce strong negative radial anisotropy given an A-type olivine fabric in the mantle wedge.…”
Section: Discussionmentioning
confidence: 99%
“…On the other hand, Ishise et al. (2018) also conduct a P‐wave radial anisotropy study of NE Japan and find negative radial anisotropy ( V PH < V PV ) in the mantle wedge and positive radial anisotropy ( V PH > V PV ) in the subducting slab. Instead of invoking different olivine types, Ishise et al.…”
Section: Discussionmentioning
confidence: 99%
“…Comparing the previous model of the top of the PHS slab (Figure S4b), the upper surface of the PHS slab is clearly shallower under the Tokyo Bay and the Boso Peninsula than the previous model. However, since only one aspect of anisotropy, azimuthal anisotropy, has been investigated in this study, it will be necessary in the future to consider vertical anisotropy (e.g., Ishise et al., 2018) and the structure of the subduction zone, including the slab structure.…”
Section: Discussionmentioning
confidence: 99%