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Kaare L. Rasmussen Hans J. F. Olsen Raymond Gwozdz Evgeniy M. Kolesnikov 《Meteoritics & planetary science》2001,36(7):1001-1006
Abstract— Jull et al. propose an alternative interpretation of our depth vs. 14C data measured on a peat core from the central Tunguska impact site (Rasmussen et al., 1999). We find that the proposed alternative is untenable. 相似文献
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Mikhalsky E. V. Alexeev N. L. Kamenev I. A. Larionov A. N. Gogolev M. A. Svetov S. A. Kunakkuzin E. L. 《Geotectonics》2020,54(3):285-307
Geotectonics - An assemblage of mafic granulites (schists), plagiogneisses, and metasedimentary rocks, which is referred to as the Filla Series, is exposed in the Rauer Islands (opposite the... 相似文献
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Geochemical and new isotopic (U-Pb, Sm-Nd) data on the Mesoproterozoic metaigneous complexes of the Rayner Province in central
East Antarctica (Enderby Land-Kemp Land and the northern Prince Charles Mountains) are presented. These territories are mainly
composed of amphibolite-to-granulite-facies orthogneisses, many of which are Y-depleted tonalite gneisses and mafic schists.
The igneous complexes of their protolith are largely products of anatexis of the lower crust; mantle-derived and upper crustal
rocks are less abundant. The geochemical features of the mafic rocks indicate that they crystallized from high-temperature
plume-related mantle melts and low-temperature lithospheric melts. As follows from the published and new Nd model ages, the
Rayner Province formed and evolved over the Paleo-to-Mesoproterozoic in the regime of accretionary and collisional tectonics
with predominance of accretion of the juvenile Paleoproterozoic crust between 1500–2400 Ma. New data show that in the northern
Prince Charles Mountains, granite-gneiss protoliths were emplaced ca. 1040 and 930 Ma ago. The Rayner Province is considered
to be a long-living mobile belt formed as a result of collision of Paleoproterozoic island-arc terranes and Archean blocks
amalgamating into a continental massif 1050–1000 Ma ago in the course of the growth of the Rodinia supercontinent. In the
northern Prince Charles Mountains, thermal processes related to magmatic underplating at the base of the crust were probably
important. 相似文献
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Charnockitic suites in central Dronning Maud Land (DML), Mac.Robertson Land (MRL), and the Bunger Hills area are compositionally varied and probably include both mantle and lower-crustal components. In this paper we present new geological and geochemical data on the DML charnockitic rocks, and compare their geochemistry with that of charnockitic rocks from several other Antarctic high-grade terranes, particularly MRL and the Bunger Hills. These areas have different geological histories and one of the main aims of this study is to investigate possible links between charnockite composition and the tectonic history of their host terranes. Antarctic charnockitic rocks form two distinct compositional groups. 510 Ma DML charnockites are relatively alkalic and ferroan, with high K2O, Zr, Ga, Fe / Mg, and Ga / Al, and very low MgO, characteristic of A-type (alkaline, commonly anorogenic) granitoids. The more mafic DML rocks, at least, were derived by fractionation of a relatively alkaline high-P–Ti ferrogabbro parent magma. Most other early Palaeozoic charnockitic rocks in Antarctica are of similar composition. In contrast, MRL (c. 980 Ma) and Bunger Hills (c. 1170 Ma) charnockites are mainly calc-alkalic or calcic and magnesian, and the associated mafic components are tholeiitic. MRL and Bunger Hills charnockites are late-orogenic, whereas DML charnockites are post-orogenic, and appear to have been emplaced after post-collision extension and decompression. These two mineralogically and geochemically distinct charnockite groups may thus reflect a compositional trend in an evolving orogen, either accretional or collisional, respectively. 相似文献
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Yoko-Dovyren层状纯橄岩-橄长岩-辉长岩地块位于西伯利亚克拉通南部的一处褶皱构造框架中(俄罗斯贝加尔湖地区北部)。该地块的结构在其厚度最大的中部得到了着重研究。剖面底部主体成分为斜长橄榄岩,并依据内部的堆晶成分变化从下往上可分为五个主要的地层序列:纯橄岩→橄长岩→橄榄辉长岩→橄榄辉长苏长岩→石英辉长苏长岩以及含易变辉石的辉长岩。该地块的矿化包括铜-镍矿化、低硫型富铂族元素(PGE)矿化以及铬铁矿化等。另外,该地块也含多种非金属矿物原材料,如硼矿化、透辉石、各种镁质硅酸盐岩等。它们也包括纯橄岩、异剥橄榄岩和橄长岩,并以较高的品质产出,有望采掘加工成为建筑材料(水泥、混凝土、沥青混凝土和建筑陶瓷)。综合利用矿物原材料可增加矿床价值,并有助于建设环保型采矿工作体系。 相似文献
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E. V. Mikhalsky 《Moscow University Geology Bulletin》2007,62(3):143-154
A review of numerous isotopic-geochronological studies is given. The major attention is paid to modern U-Pb zircon measurements using the SHRIMP method. The major tectogenesis stages recognized in the Antarctic shield are Archean (3800–3300, 3100–2800, and 2550–2450 Ma), Paleoproterozoic (2200–2000 and 1850–1700 Ma), Mesoproterozoic (1400–1250 and 1200–920 Ma), and Neoproterozoic-Early Paleozoic (600–500 Ma). Ancient Eo-and Paleoarchean processes (intrusion of tonalite gneisses protoliths, or metamorphism) took place at Enderby Land, Kemp Land, and the Prince Charles Mountains. At some localities tectonic activity ended at 1700 Ma, at other places reworking or rejuvenation occurred later. Mesoproterozoic tectogenesis was not synchronous. The completion phases of tectonic activity are known to have occurred in different places 1150, 1050, and 980–920 Ma ago. In areas of Mesoproterozoic tectogenesis, evidence of Paleoproterozoic or (rarely) Archean endogene processes is sometimes found. Most likely, this stage refers to the formation of the vast continental block. The Neoproterozoic-Early Paleozoic tectogenesis was practically synchronous over most of the Antarctic shield; on large areas it was characterized by metamorphism and pervasive schistosity, but in many other localities only various granitoids and pegmatites were intruded. Within all the areas of Neoproterozoic-Early Paleozoic tectogenesis isotopic evidence of the earlier (largely Mesoproterozoic) endogene processes are found. 相似文献
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Artyom V. Astashenok Artyom V. Yurov Sergey V. Chervon Evgeniy V. Shabanov Mohammad Sami 《Astrophysics and Space Science》2014,353(2):319-328
We develop a method for constructing exact cosmological solutions in brane world cosmology. New classes of cosmological solutions on Randall–Sandrum brane are obtained. The superpotential and Hubble parameter are represented in quadratures. These solutions have inflationary phases under general assumptions and also describe an exit from the inflationary phase without a fine tuning of the parameters. Another class solutions can describe the current phase of accelerated expansion with or without possible exit from it. 相似文献