Plio-Quaternary paleostresses in the Atlantic passive margin of the Moroccan Meseta: Influence of the Central Rif escape tectonics related to Eurasian-African plate convergence

The Atlantic Moroccan Meseta margin is affected by far field recent tectonic stresses. The basement belongs to the variscan orogen and was deformed by hercynian folding and metamorphism followed by a post-Permian erosional stage, producing the flat paleorelief of the region. Tabular Mesozoic and Mio-Plio-Quaternary deposits locally cover the Meseta, which has undergone recent uplift, while north of Rabat the subsidence continues in the Gharb basin, constituting the foreland basin of the Rif Cordillera.The Plio-Quaternary sedimentary cover of the Moroccan Meseta, mainly formed by aeolian and marine terraces deposits, is affected by brittle deformations (joints and small-scale faults) that evidence that this region – considered up to date as stable – is affected by the far field stresses. Striated faults are recognized in the oldest Plio-Quaternary deposits and show strike-slip and normal kinematics, while joints affect up to the most recent sediments.Paleostress may be sorted into extensional, only affecting Rabat sector, and three main compressive groups deforming whole the region: (1) ENE–WSW to ESE–WNW compression; (2) NNW–SSE to NE–SW compression and (3) NNE–SSW compression. These stresses can be attributed mainly to the NW–SE oriented Eurasian-African plate convergence in the western Mediterranean and the escape toward the SW of the Rif Cordillera. Local paleostress deviations may be related to basement fault reactivation. These new results reveal the tectonic instability during Plio-Quaternary of the Moroccan Meseta margin in contrast to the standard passive margins, generally considered stable.     

Early Ordovician (Floian) ostracods from the Cordillera Oriental,Northwest Argentina

The ostracod fauna from the Floian (Lower Ordovician) strata of the Cordillera Oriental, Argentina (Acoite Formation) are documented. One new genus Acoitella and four species are recognized, two of which are new (Nanopsis victoria sp. nov. and Conchoprimitia frequens sp. nov.). The diversity of the Early Ordovician ostracod faunas of the Central Andean Basin is evaluated. Compared with other regions, the ostracod diversity, at generic and specific level, of the Cordillera Oriental was comparatively high during the Tremadocian (nine species recorded) and comparatively low during the Floian (four species recorded). The taxonomic composition of the fauna is similar during the entire Early Ordovician of the Cordillera Oriental, where it displays a high percentage of soanellids. The Floian assemblages are characterized by the dominance of the eridostracan C. frequens sp. nov. with a high percentage of nondimorphic palaeocopids: Nanopsis and two genera of the Soanellidae family (Saltite and Acoitella gen nov.). An ostracod shell bed is described and interpreted to be a parautochthonous assemblage, as a result of transport within the same habitat. The composition of the fauna, with the presence of Saltite and Nanopsis, shows significant affinities with East Gondwana. Copyright © 2011 John Wiley & Sons, Ltd.     

The oldest record of Eothinoceratidae (Ellesmerocerida,Nautiloidea): Middle Tremadocian of the Cordillera Oriental,NW Argentina

Middle Tremadocian cephalopods from the Sierra de Mojotoro, Cordillera Oriental, NW Argentina, are assigned to Saloceras cf. sericeum (Salter) based on the siphuncle morphology and general shape of the conch. Saloceras sericeum (Salter) is known from the Upper Tremadocian and Floian of England and Wales, a region that formed part of eastern Avalonia during the Early Ordovician, located at a high southern latitude to the north of the Gondwanan margin. This is the oldest record of this genus and of the family Eothinoceratidae, and extends the geographical range of Saloceras, being the first positive record of its presence in Argentina and the Central Andean Basin. These remains are amongst the oldest cephalopods described from NW Argentina. They represent the third mid Tremadocian record of nautiloids at relatively high palaeolatitudes and away from the low latitude carbonate platform palaeoenvironments where the bulk of the earliest cephalopods resided. Copyright © 2010 John Wiley & Sons, Ltd.     

Monitoring of TDS and conductivity in groundwater in the seismically active region in NW Himalayas,India

<正>The earthquake precursors and earthquake prediction are the burning issue among the community of earth scientists and engineers. Studies of earthquake precursory phenomena since the last several decades have shown that significant geophysical and geochemical changes may occur prior to intermediate and large earthquakes (Hartmann and Levy, 2005; Yang et al, 2005;     

Silicate‐oxide mineral chemistry of mafic–ultramafic rocks as an indicator of the roots of an island arc: The Chilas Complex,Kohistan (Pakistan)

The Chilas Complex is a major lower crustal component of the Cretaceous Kohistan island arc and one of the largest exposed slices of arc magma chamber in the world. Covering more than 8000 km², it reaches a current tectonic width of around 40 km. It was emplaced at 85 Ma during rifting of the arc soon after the collision of the arc with the Karakoram plate. Over 85% of the Complex comprises homogeneous, olivine‐free gabbronorite and subordinate orthopyroxene–quartz diorite association (MGNA), which contains bodies of up to 30 km² of ultramafic–mafic–anorthositic association (UMAA) rocks. Primary cumulate textures, igneous layering, and sedimentary structures are well preserved in layered parts of the UMAA in spite of pervasive granulite facies metamorphism. Mineral analyses show that the UMAA is characterized by more magnesian and more aluminous pyroxene and more calcic plagioclase than those in the MGNA. High modal abundances of orthopyroxene, magnetite and ilmenite (in MGNA), general Mg–Fe–Al spatial variations, and an MFA plot of whole‐rock analyses suggest a calc‐alkaline origin for the Complex. Projection of the pyroxene compositions on the Wo–En–Fs face is akin to those of pyroxenes from island arcs gabbros. The presence of highly calcic plagioclase and hornblende in UMAA is indicative of hydrous parental arc magma. The complex may be a product of two‐stage partial melting of a rising mantle diaper. The MGNA rocks represent the earlier phase melting, whereas the UMAA magma resulted from the melting of the same source depleted by the extraction of the earlier melt phase. Some of the massive peridotites in the UMAA may either be cumulates or represent metasomatized and remobilized upper mantle. The Chilas Complex shows similarities with many other (supra)subduction‐related mafic–ultramafic complexes worldwide.     

Mineralogy and mineral chemistry of auriferous stream sediments from Al Wajh area, NW Saudi Arabia

A detailed ore microscopic study strengthened by fire assay data of Al Wajh stream sediments (Wadi Al Miyah, Wadi Haramil and Wadi Thalbah) in northwestern Saudi Arabia shows economic concentrations of gold in the silt fraction (40–63 μm). However, particles of extremely fine “dusty” gold (≤40 μm in size) were also identified in most stations as independent grains. The maximum gold content in the samples of Wadi Al Miyah is 13.61 wt%, which is reported for the heavy fraction (<40 μm). Maximum gold content in the heavy fractions of Wadi Haramil stream sediments amounts 6.90 g/t Au in a relatively coarse fraction (63–125 μm). It appears that the most fertile heavy fraction in gold among the analysed samples are those from Wadi Thalbah that have the highest index figure, which makes the placer gold in them more profitable from the economic point of view. The gold content in the heavy fractions of samples from Wadi Thalbah is economically high lying in the range 6.27–28.83 g/t Au, except for a sample collected at the upstream with 0.77 g/t Au. Al Wajh stream sediments (including the beach light and black sands) are also rich in Fe–Ti oxides, rutile and zircon, whereas monazite and thorite are much lesser. Mineral chemistry of magnetite indicates a distinct titanomagnetite variety (with 3.85 wt% TiO₂) which is consistent with the ore microscopic investigation. The titanomagnetite is V- and Cr-free, which indicates derivation from a more felsic source than a mafic one. No traces of U were found in zircon that sometimes bears up to 2.74 wt% Hf₂O₃. Chemical analyses of monazite show typical common contents of rare earth elements such as La, Ce, Nd and Sm. Thorite is either U-free or uranothorite varieties where the latter contains up to 31.79 wt% UO₂. One of the U-free thorite grains is Y-bearing and contains 7.13 wt% Y₂O₃.

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كيميائية المعادن من التحليل التقديري الناري لرسوبيات الوديان في منطقة الوجه- شمال غرب المملكة العربية السعودية

توضح الدراسة المجهرية للخامات المعدنية والتي تعضدها بيانات التحليل التقديري الناري لرسوبيات الوديان بمنطقة الوجه (وادي المياه، وادي حرامل، وادي ثلبة) في شمال المملكة العربية السعودية، أن هناك تركيزات اقتصادية للذهب في كسرة الغرين التي يتراوح حجمها من 40 إلى 63 ميكرومتر. في معظم الحالات المدروسة تم رصد حبيبات من الذهب الطليق متناهية الصغر (أقل أو تساوي 40 ميكروميتر). كما اتضح أيضا أن أعلى محتوى لفلز الذهب وجد في القطفات المعدنية الثقيلة دقيقة الحجم المأخوذة من وادي المياه والتي تقدر 13.61 جرام/الطن. أما المحتوى الأعلى في القطفات المعدنية الثقيلة الأكبر نسبيا في الحجم (تتراوح من 63 إلى 125 ميكروميتر) المأخوذة من الرواسب الوديانية بوادي حرامل يصل إلى 6.90 جرام/طن. ويبدو أن القطفات الثقيلة لرسوبيات وادي ثلبة الوديانية هي الأخصب من حيث محتوى الذهب وتلك العينات لها شكل مميز مما يجعل ذهب المراقد بذلك الوادي ذو ربحية مشجعة وذلك من الناحية الاقتصادية. وتتراوح التركيزات الاقتصادية للذهب في عينات وادي ثلبة بين 6.27 - 28.83 جرام/طن باستثناء عينة وحيدة تم تسجيل كمية ذهب بها لا تتعدى 0.77 جرام/طن. عينات الرواسب الوديانية بمنطقة الوجه (بما في ذلك الرمال الشاطئية السوداء والفاتحة اللون) غنية بمعادن خامات أكاسيد الحديد والتيتانيوم والروتيل والزيركون، بالإضافة إلى كميات أقل بكثير من معدني المونازيت والثوريت. وتوضح كيمياء المعادن أن معدن الماجنيتيت غني بالتيتانوماجنيتيت (ماجنيتيت تيتاني به 3.85% من ثاني أوكسيد التيتانيوم) وهو ما أثبتته أيضا الدراسة المجهرية. وهذا الماجنيتيت التيتاني لا يحتوي على عنصري الكروم والفاتيديوم مما يعطي دلالة على أن هذه الصخور فلسية أكثر منها مافية، وأن الزيركون الموجود لا يحتوي على عنصر اليورانيوم بينما يحتوي على أكسيد هافتيوم حتى 2.74%. أما التحاليل الكيميائية للمونازيت فإنها تظهر وجود كميات من العناصر الأرضية النادرة مثل اللانثاتوم والسيريوم والنيوديوم والسماريوم. أما معدن الثوريت فقد تم تسجيل نوعان منه أحدهما لا يحتوي على اليورانيوم أما الآخر فيحتوي على 31.79% من ثاني أوكسيد اليورانيوم. ولقد اكتشف في إحدى حبيبات الثوريت أنها لا تحتوي على اليورانيوم ولكنها تحتوي على عنصر أكسيد الأيتريوم تصل نسبته إلى 7.13%.

     

苏丹国水利水电大坝勘察的几点体会

近两年,我单位在苏丹国先后完成Kajbar,Shrerik、Sabloka、Dal、Dagash,Mograt等水利水电大坝的勘查工作,通过6个大坝的详细勘察,我们形成了一整套比较完好的国外施工经验和管理经验。本文就Kajbar大坝施工和其它大坝经验,对国外施工的准备阶段到施工阶段作业步骤做一简单的总结,并提出对国外员工管理的一点心得。     

PEDOGENESIS IN LATE PREHISTORIC INDIAN MOUNDS,UPPER MISSISSIPPI VALLEY

Inceptisols are developed on silt loam, loam, and sandy loam Indian mounds at the Keller Mound Group and Bluff Top Mound in northeastern Iowa. The mounds date to the Allamakee Phase of the Late Woodland Period (ca. 1650–1250 B.P.) and are built with fill obtained from the A, E, and upper B horizons of pre-existing soils (Alfisols). Differences in the morphologic and chemical characteristics of soils on different mounds are attributed to textural differences of the mounds' fill. Coarse-textured mound fill is pedogenically altered at a faster rate than fine-textured fill, but total carbon percentage of the A horizon attains a steady state faster in fine-textured mound fill. Total phosphorus content is used to determine from which horizons of pre-existing soils the specific layers of mound fill originated. Rates and pathways of pedogenesis in mound fill may not provide good analogues for the early stages of soil development in materials that have not undergone previous weathering and subsequent modification by humans. Nevertheless, mound soils are useful benchmarks for some pedologic studies since they provide time lines for evaluating minimum rates for development of argillic and albic horizons, as well as attainment of the Alfisol order.     

Messinian palaeoclimate and palaeo-environment in the western Mediterranean realm: insights from the geochemistry of continental deposits of NW Sardinia (Italy)

To evaluate the palaeo-environmental parameters of a portion of the Sardinia–Corsica microplate during the Messinian drop in sea level, we examined the chemistry and mineralogy of upper Tortonian–lower Messinian (late Miocene) clayey continental deposits from NW Sardinia. Differences exist between the uppermost part of the succession, which is devoid of carbonate phases, and the lower part, reflecting changes in provenance and climate. The carbonate-free samples were probably derived from quartzite of the metamorphic basement and were deposited under a climate characterized by alternating dry and relatively wet periods. The other samples were derived from basement phyllite and were deposited under a warm, dry climate that promoted the capillary rise of Ca²⁺ and bicarbonate from a shallow water table, and therefore, the precipitation of carbonate. This part of the succession contains both calcite and dolomite. The presence of barite indicates an important concentration of SO₄ ^2? in the solution from which the CaMg(CO₃)₂ precipitated. The formation of dolomite under hypersaline conditions may be explained by bacterial degradation of organic matter, which produced CO₂ and ammonia, thereby increasing the solution alkalinity. The succession formed in an oxic environment, except for a calcite-rich level that formed under relatively reducing conditions. For this level, the large amount of calcite and the lack of dolomite indicate an alkaline environment and a very low Mg²⁺/Ca²⁺ ratio in the soil solution. These observations, coupled with the reducing conditions, indicate the availability of large amounts of degraded organic matter, probably related to a period typified by a wetter climate.