南大别黄镇低温榴辉岩多同位素体系年代学研究   总被引：10，自引：0，他引：10  

陈道公  E.Deloule  程昊  夏群科  吴元保 《中国科学D辑》2003,33(9):828-840

首次对南大别黄镇低温榴辉岩和围岩花岗片麻岩进行了锆石U/Pb热电离质谱(TIMS)和二次离子质谱(SIMS)定年、云母和角闪石⁴⁰Ar-³⁹Ar定年和矿物内部Sm-Nd同位素体系研究. 一个榴辉岩样品锆石U-Pb SIMS权平均年龄为231.6±9.7 Ma, 云母的⁴⁰Ar-³⁹Ar等时年龄为232.6±2.1 Ma, 最低坪年龄为221.7±2.4 Ma; 另一榴辉岩锆石U-Pb TIMS一致年龄为221.3±1.4~222.5±2.3 Ma, 围岩花岗片麻岩锆石SIMS下交点年龄为221±35 Ma. 退变质角闪岩中角闪石⁴⁰Ar-³⁹Ar等时年龄为205.9±1.0 Ma. 除云母可能含有过剩氩外, 上述各年龄代表了低温榴辉岩峰期变质作用和退变质作用时间. 南大别黄镇低温榴辉岩变质时代不同于北大别北部熊店低温榴辉岩, 它和南大别高温榴辉岩同属统一的南大别高压-超高压地体, 高温榴辉岩和低温榴辉岩的区别可能在于它们不同的俯冲深度或折返时不同的冷却速率.  相似文献   

大别山碰撞后火山岩的锆石U-Pb年龄和氧同位素组成   总被引：11，自引：0，他引：11  

夏群科  郑永飞  E.Deloule 《高校地质学报》2003,9(2):163-171

利用阴极发光技术 (CL)观察了大别山碰撞后玄武岩和安山岩的锆石内部结构 ,并通过离子探针技术 (SIMS)测定了其U Pb年龄和氧同位素组成。玄武岩中锆石都是直接从玄武质岩浆中结晶的岩浆锆石 ,其年龄为 130± 2Ma(1σ) ;安山岩中有两种锆石 ,绝大多数是直接从安山质岩浆中结晶出来的岩浆锆石 ,年龄为 133± 3Ma(1σ) ,少数是残留的原岩锆石 ,其年龄有两组 :76 8～80 5Ma和 182 7～ 1873Ma。玄武岩和安山岩的岩浆锆石年龄表明 ,大别山碰撞后火山岩的主体应形成于 130Ma左右 ,属早白垩世。结合文献资料来看 ,大别山碰撞后火山岩和侵入岩无论是化学组成、微量元素配分、Sr Nd同位素比值还是年龄 ,都是基本一致的 ,说明火山岩和侵入岩的源区以及成因可能是相同的。玄武岩和安山岩的岩浆结晶年龄一致 ,暗示着它们之间的可能的成因联系。玄武岩锆石相对于正常地幔亏损18O(δ18O =(4 .1± 0 .6 )‰ ) ,说明其岩浆源区可能含有一定数量的俯冲板块断离后进入该区地幔的大别山榴辉岩原岩组分。安山岩中残留的原岩锆石既有扬子板块的年龄信息 ,又有华北板块的年龄信息 ,这表明华北和扬子的深部界线可能就在北淮阳  相似文献   

Geodynamic significance of the Raspas Metamorphic Complex (SW Ecuador): geochemical and isotopic constraints     

Delphine Bosch  Piercarlo Gabriele  Henriette Lapierre  Jean-Louis Malfere  Etienne Jaillard   《Tectonophysics》2002,345(1-4)

The Raspas Metamorphic Complex of southwestern Ecuador is regarded as the southernmost remnant of oceanic and continental terranes accreted in the latest Jurassic–Early Cretaceous. It consists of variably metamorphosed rock types. (1) Mafic and ultramafic rocks metamorphosed under high-pressure (HP) conditions (eclogite facies) show oceanic plateau affinities with flat REE chondrite-normalized patterns, Nd_{150 Ma} ranging from +4.6 to 9.8 and initial Pb isotopic ratios intermediate between MORB and OIB. (2) Sedimentary rocks metamorphosed under eclogitic conditions exhibit LREE enriched patterns, strong negative Eu anomalies, Rb, Nb, U, Th, Pb enrichments, low Nd_{150 Ma} values (from −6.4 to −9.5), and high initial ⁸⁷Sr/⁸⁶Sr and ^206,207,208Pb/²⁰⁴Pb isotopic ratios suggesting they were originally sediments derived from the erosion of an old continental crust. (3) Epidote-bearing amphibolites show N-MORB affinities with LREE depleted patterns, LILE, Zr, Hf and Th depletion, high Nd_{150 Ma} (>+10) and low initial Pb isotopic ratios.The present-day well defined internal structure of the Raspas Metamorphic Complex seems to be inconsistent with the formerly proposed interpretation of a “tectonic mélange”. The association of oceanic plateau rocks and continent-derived sediments both metamorphosed in HP conditions suggests that the thin edge of the oceanic plateau first entered the subduction zone and dragged sediments downward of the accretionary wedge along the Wadatti–Benioff zone. Subsequently, when its thickest part arrived into the subduction zone, the oceanic plateau jammed the subduction processes, due to its high buoyancy.In Ecuador and Colombia, the latest Jurassic–Early Cretaceous suture involves HP oceanic plateau rocks and N-MORB rocks metamorphosed under lower grades, suggesting a composite or polyphase nature for the latest Jurassic–Early Cretaceous accretionary event.  相似文献   

Aqueous alteration in the Northwest Africa 817 (NWA 817) Martian meteorite     

Ph. Gillet  J.A. BarratE. Deloule  M. WadhwaA. Jambon  V. SautterB. Devouard  D. NeuvilleK. Benzerara  M. Lesourd 《Earth and Planetary Science Letters》2002,203(1):431-444

Samples of a new Martian meteorite of the nakhlite family (NWA 817) contain traces of an iron-rich alteration product. Textural arguments indicate that this alteration product has been formed on the parent body of the meteorite (Mars). The chemical composition and structural data (X-ray diffraction, transmission electron microscopy and vibrational spectroscopy) show that the alteration mineral is a hydrous phase from the smectite family. Major elements and rare earth elements suggest that the formation of the alteration phase is related to the circulation of an aqueous fluid which composition is controlled by the dissolution of feldspars to account for a positive Eu anomaly, olivine and possibly apatite. Hydrogen isotope data display negative δD values ranging from −60 to −280‰ in olivine and pyroxenes and from −140 to −181‰ in the alteration phase. The values of δD for the alteration product show a small scatter with a mean value of −170±14‰. These values are lower than those previously obtained on other Martian meteorites, which give mainly positive δD values. These positive values have been interpreted as resulting from the interaction of the Martian meteorites with water from the Martian atmosphere. Ruling out the effect of terrestrial alteration, it is suggested that alteration in the NWA 817 meteorite was likely produced on Mars by the circulation of an aqueous fluid originating from a chemical reservoir, such as the Martian mantle, which has not equilibrated with a fractionated Martian atmosphere.  相似文献   

北大别黄土岭麻粒岩锆石U—Pb离子探针定年   总被引：28，自引：6，他引：28  

吴元保  陈道公  夏群科  Etienne DELOULE  程昊 《岩石学报》2002,18(3):378-382

阴极发光显微结构分析表明 ,北大别黄土岭麻粒岩中存在三种类型的锆石 :原岩锆石、麻粒岩相锆石和残留锆石。对它们分别进行离子探针定年 ,得到黄土岭麻粒岩的原岩年龄约为 2 70 0 Ma、麻粒岩相变质事件的年龄为 2 0 5 2± 10 0 Ma、残留锆石的年龄为约 3.4 Ga。以上研究表明黄土岭麻粒岩为残存的扬子板块的结晶基底 ,而约 3.4 Ga残留锆石的发现 ,则首次证明大别山地区存在古太古代的陆壳物质  相似文献   

Late Holocene local vegetation dynamics in the marsh of Gravgaz(southwest Turkey)     

Marleen Vermoere  Thijs Van Thuyne  Simon Six  Leo Vanhecke  Marc Waelkens  Etienne Paulissen  Erik Smets 《Journal of Paleolimnology》2002,27(4):429-451

Late Holocene local vegetation succession is reconstructed in twodifferent sites in a small-scale open marsh ecosystem in southwest Turkey.This is done by comparison of the fossil local pollen assemblage zones in twocores with the local pollen data of 40 surface samples from the marsh. Thepollen data are supplemented with sedimentological and archaeological data. Theinsertion of the mean pollen data of the local pollen zones as passive samplesinto the canonical correspondence analysis triplot of the modern samples allowsus to detect modern analogues for the fossil pollen zones. From this numericalcomparative approach it is concluded that the marsh area was relatively dryuntil ca 2500 BP. After 2500 BP the area shifts towards a wet area dominated bySparganium and/or Typha angustifolia. A diversification of the marsh vegetationstarts at ca 2400/2300 BP. The area around one core site seems to have beensituated in an area with slowly flowing source water, whereas the other coresite is likely to have been characterised by damp conditions. The steadilyincreasing dryness of the marsh area starts after ca 680 BP. The drying upappears to be associated with recent agricultural and grazing pressure.  相似文献   

Experimental study on the flow around two tandem cylinders with unequal diameters     

Yangyang Gao  Stephane Etienne  Xikun Wang  Soon Keat Tan 《中国海洋大学学报(英文版)》2014,13(5):761-770

In this paper, flow around two circular cylinders in tandem arrangement with unequal diameters has been investigated using the particle image velocimetry technique (PIV) in a water channel. The upstream to downstream diameter ratio was kept constant at d/D = 2/3, the centre-to-centre distance was varied from 1.2D to 5D and the Reynolds number was varied from 1200 to 4800. The flow characteristics were analyzed through ensemble-averaged patterns of velocity, vorticity, normalized Reynolds stress contours and streamlines. Based on ensemble-averaged and instantaneous flow fields, different flow patterns, including single-wake-shedding at small spacing ratio, bi-stable flow behavior (alternating behavior of reattachment and vortex shedding) at intermediate spacing ratio and co-shedding pattern at large spacing ratio were observed. The effects of Reynolds number and the centre-to-centre spacing ratio on flow patterns and turbulent characteristics were also investigated. It was found that the diameter ratio appears to have a certain effect on the flow patterns at intermediate spacing ratios, where the reattachment of shear layer depends on the lateral width of the wake flow in the lee of the upstream cylinder. Extensive discussion on the distributions of Reynolds stress and turbulent kinetic energy was presented.  相似文献   

V oxidation state in Fe–Ti oxides by high-energy resolution fluorescence-detected X-ray absorption spectroscopy     

Amélie Bordage  Etienne Balan  Johan P. R. de Villiers  Robert Cromarty  Amélie Juhin  Claire Carvallo  Georges Calas  P. V. Sunder Raju  Pieter Glatzel 《Physics and Chemistry of Minerals》2011,38(6):449-458

The oxidation state of vanadium in natural and synthetic Fe–Ti oxides is determined using high-energy resolution fluorescence-detected X-ray absorption spectroscopy (HERFD-XAS). Eleven natural magnetite-bearing samples from a borehole of the Main Magnetite Layer of the Bushveld Complex (South Africa), five synthetic Fe oxide samples, and three natural hematite-bearing samples from Dharwar supergroup (India) are investigated. V K edge spectra were recorded on the ID26 beamline at the European Synchrotron Radiation Facility (Grenoble, France), and the pre-edge features were used to determine the local environment and oxidation state of vanadium. In the case of the magnetite samples (natural and synthetic), we show that vanadium is incorporated in the octahedral site of the spinel structure under two oxidation states: +III and +IV. The variations of the pre-edge area are interpreted as various proportions in V³⁺ and V⁴⁺ (between 9.5 and 16.3% of V⁴⁺), V³⁺ being the main oxidation state. In particular, the variations of the V⁴⁺/V³⁺ ratio along the profile of the Main Magnetite Layer seem to follow the crystallization sequence of the layer. In the case of the hematite samples from India, the pre-edge features indicate that vanadium is substituted to Fe and mainly incorporated as V⁴⁺ (between 40 and 72% of V⁴⁺). We also demonstrate the potentiality of HERFD-XAS for mineralogical studies, since it can filter out the unwanted fluorescence and give better resolved spectra than conventional XAS.  相似文献   

“Stones from the dangerous winds”: reef platform mega-clasts in the tropical Pacific Islands     

James P. Terry  Samuel Etienne 《Natural Hazards》2011,56(3):567-569

Tsunamis and intense tropical storms compete as viable mechanisms for catastrophic marine inundations of coastlines, and so interpretation of deposits laid down by palaeo-events is often problematic. Here, examples are presented from the tropical South Pacific Islands to demonstrate how indigenous knowledge may provide vital clues supporting sedimentological investigation and thereby helping to explain the origin of giant boulders emplaced on top of coral reef platforms.  相似文献   

Deciphering the weathering processes using environmental mineralogy and geochemistry: Towards an integrated model of laterite and podzol genesis in the Upper Amazon Basin     

Emmanuel Fritsch  Etienne Balan  Nadia Régina Do Nascimento  Thierry Allard  Marion Bardy  Guilherme Bueno  Sylvie Derenne  Adolpho José Melfi  Georges Calas 《Comptes Rendus Geoscience》2011,343(2-3):188-198

This article reports major results from collaborative research between France and Brazil on soil and water systems, carried out in the Upper Amazon Basin. It reveals the weathering processes acting in the partly inundated, low elevation plateaus of the Basin, mostly covered by evergreen forest. Our findings are based on geochemical data and mineral spectroscopy that probe the crystal chemistry of Fe and Al in mineral phases (mainly kaolinite, Al- and Fe-(hydr)oxides) of tropical soils (laterites). These techniques reveal crystal alterations in mineral populations of different ages and changes of metal speciation associated with mineral or organic phases. These results provide an integrated model of soil formation and changes (from laterites to podzols) in distinct hydrological compartments of the Amazon landscapes and under altered water regimes.  相似文献