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431.
本文通过大比例尺野外测量及镜下观察,对鲁西寒武系第三统张夏组的附枝菌与附枝菌微生物灰岩特征进行了详细研究。附枝菌是一种树枝状蓝细菌,一般向上生长扩展,形成灌木状附枝菌群落,生长于附枝菌微生物丘内部。而在微生物丘的外部边缘,附枝菌群落呈半闭合的房室状,与肾状菌十分相似。房室状附枝菌群落可能是在微生物丘外部边缘受局部高能微环境(如水流、波浪等)的影响形成的。在其形成后,其保存状态则是由附枝菌的钙化作用及早期成岩作用决定。由于附枝菌构成其微生物岩的生长骨架,且该微生物岩不具备清晰的中型构造,故可称其为附枝菌格架岩,作为对微生物岩分类命名的又一补充。附枝菌格架岩一般生长于台地边缘或台地外部斜坡环境,其生长过程受水动力条件、阳光照射及海水清澈度等影响。  相似文献   
432.
Voluminous granitic intrusions are distributed in the West Junggar, NW China, and they can be classified as the dioritic rocks, charnockite and alkali-feldspar granite groups. The dioritic rocks (SiO2 = 50.4–63.8 wt.%) are calc-alkaline and Mg enriched (average MgO = 4.54 wt.%, Mg# = 0.39–0.64), with high Sr/Y ratios (average = 21.2), weak negative Eu (average Eu/Eu = 0.80) and pronounced negative Nb–Ta anomalies. Their Sr–Nd and zircon Hf isotopic compositions ((87Sr/86Sr)i = 0.7035–0.7042, εNd(t) = 4.5–7.9, εHf(t) = 14.1–14.5) show a depleted mantle-like signature. These features are compatible with adakites derived from partial melting of subducted oceanic crust that interacted with mantle materials. The charnockites (SiO2 = 60.0–65.3 wt.%) show transitional geochemical characteristics from calc-alkaline to alkaline, with weak negative Eu (average Eu/Eu = 0.75) but pronounced negative Nb–Ta anomalies. Sr–Nd and zircon Hf isotopic compositions ((87Sr/86Sr)i = 0.7037–0.7039, εNd(t) = 5.2–8.0, εHf(t) = 13.9–14.7) also indicate a depleted source, suggesting melts from a hot, juvenile lower crust. Alkali-feldspar granites (SiO2 = 70.0–78.4 wt.%) are alkali and Fe-enriched, and have distinct negative Eu and Nb–Ta anomalies (average Eu/Eu = 0.26), low Sr/Y ratios (average = 2.11), and depleted Sr–Nd and zircon Hf isotopic compositions ((87Sr/86Sr)i = 0.7024–0.7045, εNd(t) = 5.1–8.9, εHf(t) = 13.7–14.2). These characteristics are also comparable with those of rocks derived from juvenile lower crust. Despite of the differences in petrology, geochemistry and possibly different origins, zircon ages indicate that these three groups of rocks were coevally emplaced at ~ 305 Ma.A ridge subduction model can account for the geochemical characteristics of these granitoids and coeval mafic rocks. As the “slab window” opened, upwelling asthenosphere provided enhanced heat flux and triggered voluminous magmatisms: partial melting of the subducting slab formed the dioritic rocks; partial melting of the hot juvenile lower crust produced charnockite and alkali-feldspar granite, and partial melting in the mantle wedge generated mafic rocks in the region. These results suggest that subduction was ongoing in the Late Carboniferous and, thus support that the accretion and collision in the Central Asian Orogenic Belt took place in North Xinjiang after 305 Ma, and possibly in the Permian.  相似文献   
433.
In the present paper the intensity of serration of quartz grain boundary sutures in the Palaeoproterozoic age Malanjkhand granite (Central India) is quantified using the ruler method of fractal analyses. The northern margin of the granite has proximity to the Central Indian Suture (CIS) that forms the southernmost part of Central Indian Tectonic Zone (CITZ) along which amalgamation of the northern and southern Indian shields took place. The fractal dimension (D) of the quartz sutures is calculated in 13 samples collected at varying distance from the CIS. D values are noted to increase in samples towards the CIS. This demonstrates the influence of the tectonic events along the CIS on fabric development in the Malanjkhand granite. Magmatic fabric defined by preferentially oriented feldspar laths and high-T solid-state deformation fabrics are observed in areas distant from the CIS. In contrast, mylonites and low-T fabrics such as bulging quartz grain boundaries occur in proximity to the CIS. It is inferred that the emplacement and high-T fabric development in the Malanjkhand granite was synchronous with regional accretionary processes that occurred in the region during the Palaeoproterozoic. Two different possibilities, one involving a single tectonic event and the other involving multiple tectonic events are discussed to explain the superimposition of low-T over high-T fabric due to which intensity of quartz grain boundary serration increases towards the CIS.  相似文献   
434.
Alluvial and colluvial gem sapphires are common in the basaltic fields of the French Massif Central (FMC) but sapphire-bearing xenoliths are very rare, found only in the Menet trachytic cone in Cantal. The O-isotope composition of the sapphires ranges between 4.4 and 13.9‰. Two distinct groups have been defined: the first with a restricted isotopic range between 4.4 and 6.8‰ (n = 22; mean δ18O = 5.6 ± 0.7‰), falls within the worldwide range defined for blue-green-yellow sapphires related to basaltic gem fields (3.0 < δ18O < 8.2‰, n = 150), and overlaps the ranges defined for magmatic sapphires in syenite (4.4 < δ18O < 8.3‰, n = 29). A second group, with an isotopic range between 7.6 and 13.9‰ (n = 9), suggests a metamorphic sapphire source such as biotite schist in gneisses or skarns. The δ18O values of 4.4–4.5‰ for the blue sapphire-bearing anorthoclasite xenolith from Menet is lower than the δ18O values obtained for anorthoclase (7.7–7.9‰), but suggest that these sapphires were derived from an igneous reservoir in the subcontinental spinel lherzolitic mantle of the FMC. The presence of inclusions of columbite-group minerals, pyrochlore, Nb-bearing rutile, and thorite in these sapphires provides an additional argument for a magmatic origin. In the FMC lithospheric mantle, felsic melts crystallized to form anorthoclasites, the most evolved peraluminous variant of the alkaline basaltic melt. The O-isotopic compositions of the first group suggests that these sapphires crystallized from felsic magmas under upper mantle conditions. The second group of isotopic values, typified for example by the Le Bras sapphire with a δ18O of 13.9‰, indicates that metamorphic sapphires from granulites were transported to the surface by basaltic magma.  相似文献   
435.
A detailed palaeomagnetic study of Cretaceous age volcanic and sedimentary arc rocks from central Cuba has been carried out. Samples from 32 sites (12 localities) were subjected to detailed demagnetisation experiments. Nineteen sites from the Los Paso, Mataguá, Provincial and Cabaiguán Formations yielded high unblocking temperature, dual polarity directions of magnetisation which pass the fold tests with confidence levels of 95% or more and are considered to be primary in origin. The palaeomagnetic inclinations are equivalent to palaeolatitudes of 9°N for the Aptian, 18°N for the Albian. A synfolding remanence identified in 5 sites from the younger Hilario Formation indicates a late Cretaceous remagnetisation at a palaeolatitude of 16°N. Our results are in good agreement with previous palaeogeographic models and provide the first high quality palaeomagnetic data demonstrating the gradual northward movement of the Cretaceous Volcanic Arc throughout the Cretaceous. The declination values obtained all indicate significant and similar amounts of anticlockwise rotation from the oldest sequences studied through to the late Cretaceous remagnetisation. This rotation is most likely related to collision of the arc with the North American plate and transpressional strike slip movement along the northern margin of the Caribbean plate as it progressed eastwards into the large Proto-Caribbean basin.  相似文献   
436.
The Chaco foreland basin was initiated during the late Oligocene as a result of thrusting in the Eastern Cordillera in response to Nazca–South America plate convergence. Foreland basins are the result of the flexural isostatic response of an elastic plate to orogenic and/or thrust sheet loading. We carried out flexural modelling along a W–E profile (21.4°S) to investigate Chaco foreland basin development using new information on ages of foreland basin strata, elastic and sedimentary thicknesses and structural histories. It was possible to reproduce present-day elevation, gravity anomaly, Moho depth, elastic thicknesses, foreland sedimentary thicknesses and the basin geometry. Our model predicted the basin geometry and sedimentary thicknesses for different evolutionary stages. Measured thicknesses and previously proposed depozones were compared with our predictions. Our results shed more light on the Chaco foreland basin evolution and suggest that an apparent decrease in elastic thickness beneath the Eastern Cordillera and the Interandean Zone could have occurred between 14 and 6 Ma.  相似文献   
437.
山东沂水杂岩由新太古代岩浆杂岩和中太古代的变质杂岩组成,其后者中的变基性岩石,特别是基性麻粒岩,常与紫苏花岗岩紧密伴生,而且多呈大小不等的包体或呈层状体产出。本文主要对变基性岩进行岩石地球化学和锆石SHRIMP UPb定年研究。根据岩石学特征,可将变基性岩分为三类:含紫苏辉石斜长角闪岩、含石榴子石角闪二辉斜长麻粒岩和含尖晶石—石榴子石的角闪二辉麻粒岩。它们原岩分别为安山质玄武岩、高铁镁质玄武岩和玄武质科马提岩(?)。三类岩石稀土元素和微量元素配分有一定差别:第一类含紫苏辉石斜长角闪岩富集轻稀土和大离子亲石元素,亏损Nb、Ta、Zr、Hf等高场强元素;后二类麻粒岩相变质岩的稀土配分模式为近平坦型或轻稀土略为富集, K、Rb、Ba等元素也轻微富集,其他元素与MORB的比值接近于1。变基性岩中锆石定年结果显示有四组年龄值,其中2719Ma和2560~2607Ma分别代表早期麻粒岩相变质作用的年龄下限和上限;2509~2522Ma代表另一期角闪岩相—麻粒岩相变质作用的时代,发生在沂水岩浆杂岩侵入之后;2485Ma和2497Ma代表与流体作用有关的变质作用和新生锆石的形成年龄。  相似文献   
438.
中亚地区中生代以来的地貌巨变与岩石圈动力学   总被引:3,自引:1,他引:2       下载免费PDF全文
王清晨 《地质科学》2009,44(3):791-810
中亚地区的地貌自中生代以来发生过两次巨变:一次是青藏高原的隆起,另一次是中生代中国东部高原及其西侧共存的中亚准平原的兴衰。青藏高原的隆起引起了全球气候和中亚环境的巨变。对此,自80年代以来开展的国际合作已经在地质学和地球物理学等研究领域取得了丰硕的成果。不过,在解释高原隆升-气候变化-剥蚀作用的相互关系方面仍存歧见。相比之下,中亚地区中生代的地貌巨变尚属新的研究课题。人们认识到,中亚地区在中侏罗世至新近纪曾存在一个准平原,而在中国东部则存在一个中生代高原。这一中生代地貌巨变引发出许多新的思考,如:为什么这一中生代准平原能保存长达150 Ma?中国东部高原是怎样形成的,又是怎样消失的?这两次地貌巨变及其相关的岩石圈动力学将是“TOPO?CENTRAL?ASIA”这一国际岩石圈计划项目的研究主题。  相似文献   
439.
随着山东省工业化进程的加快发展,矿产的开发存在一系列问题,尤其监管科技手段不高,为了解决以上问题,山东省自然资源厅启动了山东省矿产资源网格化监管系统的建设,综合运用地理信息系统(简称GIS)、物联网、三维仿真、视频监控等技术,构建了省、市、县、矿山四级互联互通的网格化监管体系,针对全省露天开采矿山、重点地下开采矿山和卤水等液体矿山等矿产资源进行人员定位、视频、产量、流量等实时化、动态化监管,建立了全省矿产资源开发利用"天上看、地上查、地下控、网上管"的立体监管格局,增强监督管理水平、有效抑制非法违法开采行为。  相似文献   
440.
The interaction between the land surface and the atmosphere is a crucial driver of atmospheric processes. Soil moisture and precipitation are key components in this feedback. Both variables are intertwined in a cycle, that is, the soil moisture – precipitation feedback for which involved processes and interactions are still discussed. In this study the soil moisture – precipitation feedback is compared for the sempiternal humid Ammer catchment in Southern Germany and for the semiarid to subhumid Sissili catchment in West Africa during the warm season, using precipitation datasets from the Climate Hazards Group InfraRed Precipitation with Station data (CHIRPS), from the German Weather Service (REGNIE) and simulation datasets from the Weather Research and Forecasting (WRF) model and the hydrologically enhanced WRF-Hydro model. WRF and WRF-Hydro differ by their representation of terrestrial water flow. With this setup we want to investigate the strength, sign and variables involved in the soil moisture – precipitation feedback for these two regions. The normalized model spread between the two simulation results shows linkages between precipitation variability and diagnostic variables surface fluxes, moisture flux convergence above the surface and convective available potential energy in both study regions. The soil moisture – precipitation feedback is evaluated with a classification of soil moisture spatial heterogeneity based on the strength of the soil moisture gradients. This allows us to assess the impact of soil moisture anomalies on surface fluxes, moisture flux convergence, convective available potential energy and precipitation. In both regions the amount of precipitation generally increases with soil moisture spatial heterogeneity. For the Ammer region the soil moisture – precipitation feedback has a weak negative sign with more rain near drier patches while it has a positive signal for the Sissili region with more rain over wetter patches. At least for the observed moderate soil moisture values and the spatial scale of the Ammer region, the spatial variability of soil moisture is more important for surface-atmosphere interactions than the actual soil moisture content. Overall, we found that soil moisture heterogeneity can greatly affect the soil moisture – precipitation feedback.  相似文献   
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