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JournalISSN: 1819-7140

Russian Journal of Pacific Geology 

Springer Science+Business Media
About: Russian Journal of Pacific Geology is an academic journal published by Springer Science+Business Media. The journal publishes majorly in the area(s): Volcanic rock & Geology. It has an ISSN identifier of 1819-7140. Over the lifetime, 672 publications have been published receiving 3004 citations. The journal is also known as: Tikhookeanskaya geologiya.


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Journal ArticleDOI
TL;DR: In this article, geochronological and geochemical determinations are analyzed to identify the Albian-Cenomanian continental-margin orogenic belt and simultaneous igneous province of Pacific Asia.
Abstract: Geological data and about 300 precision geochronological and geochemical determinations are analyzed to identify the Albian–Cenomanian continental-margin orogenic belt and simultaneous igneous province of Pacific Asia. The orogenic belt represents a newly formed region of continental lithosphere that resulted from the deformation of mainly Jurassic–Early Cretaceous epioceanic terranes. The igneous province is made up of volcanic and intrusive complexes of mostly Albian age, which are syn-orogenic within the belt and post-orogenic beyond it. The igneous rocks include A-, I-, and S-type granitoids; adakites; and VAB- and OIB-type basalts and their intrusive analogues. Both the orogenic belt and the igneous province were formed in a tectonic setting of a transform continental margin between 110 and 95 Ma. The interval of 103–97 Ma became the peak of orogenic and magmatic activity caused by upwelling of the hot asthenospheric mantle through destructed stagnant slabs of the pre-Albian subduction. The Albian–Cenomanian age of the large gold, copper, tungsten, tin, and other ore deposits argues in favor of recognition of the corresponding metallogenic province. The first age data (100–97 Ma) are reported for the granite from the Malmyzh deposit within the Sikhote-Alin Ridge.

46 citations

Journal ArticleDOI
TL;DR: A massif of porhyritic microcline biotite granites located in the southern part of the Bureya (Turan) terrane has an age of 185 ± 1 Ma as discussed by the authors.
Abstract: A massif of porhyritic microcline biotite granites located in the southern part of the Bureya (Turan) terrane has an age of 185 ± 1 Ma. The granites are characterized by (K2O + Na2O) > 8%, a K2O predominance over Na2O, and a moderately differentiated REE distribution pattern ((La/Yb)n = 14.7–28.5). The obtained age indicates that at least one stage of the Early Mesozoic granitoid magmatism in the Bureya terrane occurred in the Early Jurassic. The formation of early Mesozoic granitoids was presumably related to collision between North Asian and Sino-Korean cratons, and the intervening Amur superterrane, although a subduction origin also cannot be completely ruled out.

34 citations

Journal ArticleDOI
TL;DR: The spatial-genetic relationships between transit fault systems of the East Asian global shear zone (EAGSZ) are analyzed in this paper, where it is shown that the internal structure between the Okhotsk and South China seas is identical to that of world-known natural and experimental shear zones, which confirms its development as an integral structure.
Abstract: The spatial-genetic relationships between transit fault systems of the East Asian global shear zone (EAGSZ) are analyzed. It is established that the EAGSZ internal structure between the Okhotsk and South China seas is identical to that of world-known natural and experimental shear zones, which confirms its development as an integral structure. The structural-kinematic analysis included the Tan-Lu-Sikhote-Alin (TS) system of left-lateral strike-slip faults (NNE 25°–30°) and the Bohai-Amur (BA) system of updip-strike-slip faults (NE 50°–70°). It is shown that these systems were formed as structural parageneses during two stages. The first and shear-thrust stage (Jurassic-Early Cretaceous) was marked by general NNW-oriented compression with the formation of the TS system of left-lateral strike-slip faults and their structural parageneses (compression structures) such as the BA system of updip-thrusts. The second, strike-slip-pull apart stage (Late Cretaceous-Cenozoic) was characterized by SE-directed tangential compression, which was generated by the SW left-lateral displacement of the continental crust along the Central Sikhote-Alin deep-seated fault. In such dynamic settings, the updip-thrust kinematics of the BA system gave way to that of left-lateral strike-slip faults. The strike-slip faults were formed in the transtension regime (shear with extension), which determined the development of pull-apart structures, where the left-lateral shear extension component played the decisive role. Simultaneously, the extension involved the Tan-Lu strike-slip fault with the formation of the rift valley and the discrete development of sedimentary basins along the latter.

28 citations

Journal ArticleDOI
TL;DR: The structure, litho-and biostratig� raphy of the East Sakhalin accretionary wedge were investigated in the central part of the Sakhali mountains along two profiles approximately 40 km long crossing the Nabil and Rymnik zones as mentioned in this paper.
Abstract: The East Sakhalin accretionary wedge is a part of the Cretaceous-Paleogene accretionary system, which developed on the eastern Asian margin in response to subduction of the Pacific oceanic plates. Its for� mation was related to the evolution of the Early Cretaceous Kem-Samarga island volcanic arc and Late Cre� taceous-Paleogene East Sikhote Alin continentalmargin volcanic belt. The structure, litho�, and biostratig� raphy of the accretionary wedge were investigated in the central part of the East Sakhalin Mountains along two profiles approximately 40 km long crossing the Nabil and Rymnik zones. The general structure of the examined part of the accretionary wedge represents a system of numerous eastvergent tectonic slices. These tectonic slices. tens to hundreds of meters thick. are composed of various siliciclastic rocks, which were formed at the convergent plate boundary, and subordinate oceanic pelagic cherts and basalts, and hemipelagic siliceous and tuffaceous-siliceous mudstones. The siliciclastic deposits include trenchfill mudstones and turbidites and draping sediments. The structure of the accretionary wedge was presumably formed owing to offscraping and tectonic underplating. The offscrape d and tectonically underplated fragments were proba� bly tectonically juxtaposed along outofsequence thrusts with draping deposits. The radiolarian fauna was used to constrain the ages of rocks and time of the accretion episodes in different parts of the accretionary wedge. The defined radiolarian assemblages were correlated with the radiolarian scale for the Tethyan region using the method of unitary associations. In the Nabil zone, the age of pelagic sediments is estimated to have lasted from the Late Jurassic to Early Cretaceous (Barremian); that of hemipelagic sediments, from the early Aptian to middle Albian; and trenchfill and draping depo sits of the accretionary complex date back to the middle-late Albian. In the Rymnik zone, the respective ages of cherts, hemipelagic sediments, and trench facies with draping deposits have been determined as Late Jurassic to Early Cretaceous (middle Albian), mid� dle Aptian-middle Cenomanian, and middle-late Cenomanian. East of the rear toward the frontal parts of the accretionary wedge, stratigraphic boundaries between sediments of different lithology become succes� sively younger. Timing of accretion episodes is based on the age of trenchfill and draping sediments of the accretionary wedge. The accretion occurred in a period lasting from the terminal Aptian to the middle Albian in the western part of the Nabil zone and in the middle Cenomanian in the eastern part of the Rymnik zone. The western part of the Nabil zone accreted synchronously with the Kiselevka-Manoma accretionary wedge located westerward on the continent. These accretionary wedges presumably formed along a single conver� gent plate margin, with the Sakhalin accretionary system located to the south of the Kiselevka-Manoma ter� rane in the Albian.

27 citations

Journal ArticleDOI
TL;DR: In this paper, geochemical studies of the Middle-Late Cenozoic succession of volcanic rocks from the northern part of the Rio Grande Rift were conducted. And they showed that basanites and alkali basalts of the territory had geochemical characteristics of sublithospheric slab and above-sl ab sources.
Abstract: Geochemical studies of the Middle—Late Cenozoic succession of volcanic rocks from the northern part of the Rio Grande Rift were conducted. The initial activation of the rift structure was coeval with voluminous eruptions of lava and pyroclastic material of mainly intermediate and acid compositions in the San Juan volcanic field 35–27 Ma. The composition of the volcanic products after the rifting was dominated by basic and intermediate lavas. It is shown that the basanites and alkali basalts of the territory had geochemical characteristics of sublithospheric slab and above–sl ab sources. The processes of the riftogenic thinning of lithosphere are expressed by geochemical parameters that reflect the interaction between the liquids from the sublithospheric mantle and the rocks from different levels of both the lithospheric mantle and lower crust. In the 35–18 Ma interval, melts of different–depth sublithospheric and lithospheric sources erupted simultaneously in the northern part of the rift. However, the products of interaction between the sublithospheric and lithospheric materials dominated later in the past 15 Ma, although the sublithospheric magmatic liquids erupted at the northern structural termination of the rift within the Yampa volcanic field at about 10 Ma.

26 citations

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No. of papers from the Journal in previous years
YearPapers
202340
202277
202130
202042
201942
201843