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- W2010441636 abstract "A horizontal buckle model is proposed for the geodynamics of Neogene clockwise rotation of the SW Japan arc and the back arc spreading of the Japan Sea. The model explains the dynamics and kinematics of the formation of megakink bands developed extensively in the Shimanto belt of the Outer Zone of SW Japan (Yanai 1986a, 1986b). Using the megakink bands as indicators of stress orientation and shortening magnitude, the regional axial trajectory () is longitudinal and almost parallel to the long axis of the SW Japan arc, and the axis is directed nearly vertical. The shortening magnitude increases up to 22%, crossing SW Japan from Japan Sea to the Philippine Sea. These data suggest that the rotation mode of SW Japan is analogous to buckle folding with vertical rotation axes, in which the external compressional force is exerted parallel to the arc trend. The SW Japan wing was moved with reference to the nearly fixed Ryukyu wing, forming the inner compression zone (intrados) on the Philippine Sea side. Sinistral strike-slip faults subparallel to the arc trend, such as Median Tectonic Line, would assist the overall buckle rotation of SW Japan arc. The addition of longitudinal push may enhance the potentially extensional stresses in the back arc region, thereby giving rise to the spreading. The most suitable candidate for the push is the propagating collisional effects of India to Eurasia. I speculate that the amalgamation and fragmentation of the Eurasian continental rim, combined with a continual supply of oceanic materials from the downgoing slab, provides the most likely geodynamic origin for back arc spreading of the Japan Sea." @default.
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- W2010441636 date "1989-09-01" @default.
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- W2010441636 title "A Horizontal Buckle Model as a Dynamic Mechanism for Back Arc Spreading of the Japan Sea" @default.
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- W2010441636 doi "https://doi.org/10.1086/629335" @default.
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