The paper focuses on reconstruction of the Ocean Plate Stratigraphy (OPS)from young orogenic belts—the Pacific Ocean Plate Stratigraphy,from the Phanerozoic accretionary complex and orogenic mélange,and also briefly introduces reconstruction of the OPS of the eastern ancient Indian Ocean (East New Tethyan Ocean)and ancient Asian Ocean. Through petrology,paleontology and stratigraphy analysis on the Mesozoic accretionary complexes of the southern Alaska,the Jurassic and early Cretaceous accretionary complexes of far east Russian and northeastern China,the Permian-Jurassic-Cretaceous accretionary complexes of Japan,the Jurassic accretionary complexes in the Philippines and the middle Jurassic-Paleocene Francesca accretionary complexes in California,the Pacific Ocean plate stratigraphy are reconstructed. The middle Jurassic-Paleocene Francesca complex in the California coastal mountains has been studied in depth. The overlying ophiolite (Grand Valley Group of the forearc basin ophiolite)in the subduction zone is effectively distinguished from the Marin Cape complex (its protolith is the mid-ocean ridge basalt)in the north of Francesca. The subduction and collision of the Pacific plate and the associated rifting and spreading of the front arc basin are also clarified. Nevertheless,the retention and episodic accretion of the plate subduction with a short lifespan may not be easily identified in the subduction system.
The paper focuses on reconstruction of the Oceanic Plate Stratigraphy (OPS)from the Precambrian accretionary complexes and mélange of ancient orogenic belts,including the Pacific OPS reconstructed from the Neoproterozoic Mona Supergroup mélange in Anglesey,Wales,United Kingdom,and the Paleo-Indian OPS reconstructed from the Early Archean Cleaverville greenstone belt,Pilbara,northwest Australia. The early Archean basalt-silicate-clastic sequence in the Marble Bar area of the East Pilbara Block of Australia is highly similar to the Permian-Triassic ocean plate strata of Japan in rock composition and geochemical characteristics. This conclusion will provide strong support for evolution of the sedimentary environments of the early Archean OPS from the high-heat flow ridge spreading area,through the hot spot,to the low-heat flow trench,terrigenous clastic depositional zone. According to the rock records of the OPS in the accretive orogenic belt,the main composition and rock types of the OPS strata from the Archean to the present are similar. Therefore,the processes of ocean spreading,deposition,subduction and accretion have not changed significantly during the Earth's 3.8-byr-history. However,the oceanic plate properties and the oceanic plate stratigraphic composition of young orogenic belts may have changed with time. Precambrian mantle temperature was slightly high,and the degree of partial melting was high in the Archean. The melting amount greatly exceeded the expansion rate of the ocean crust,so the sheet dike group did not form in ancient oceanic crust.