澳大利亚前寒武系和寒武系迭层石的分布

前言我们在澳大利亚工作的目的是检验苏联迭层石分类及其分带方案(Scheme)的可靠性。我们发现他们的分类,如在别处讨论过的一样,在我们的迭层石中一般是可应用的。我们尽可能广泛地获得了迭层石在地理和时代(temporal)上分布范围的资料。普里斯(1971)对阿得累德(Adelaide)地槽前寒武纪和寒武纪迭层石作了详细的地层和岩相研究。沃尔特(1970,1972)研究了阿马德斯(Amadeus)、乔治纳(Georgina)、麦卡阿瑟     

OBSERVATIONS ON THE QUATERNARY GEOLOGY OF THE LADAKH RANGE, NORTHWEST INDIAN HIMALAYA

OBSERVATIONS ON THE QUATERNARY GEOLOGY OF THE LADAKH RANGE, NORTHWEST INDIAN HIMALAYA     

艾比湖盐尘对周边地区土壤盐分及景观变化的影响

通过对准噶尔盆地西部艾比湖地区盐尘的扩散和堆积进行观测和取样分析,鉴别出粉尘中可溶盐的化学成分、pH和盐尘堆积强度,分析研究了盐尘的形成、分布特征和灾害强度以及盐尘暴与温度、降水、风等气候因子之间的相关关系.结果表明:近50 a来艾比湖的沉积环境总体是比较稳定的,但由于气候波动与人类活动引起艾比湖水位、水域面积曾发生较明显的变化,并产生了盐尘暴的发生、湖泊和土壤盐度以及湖周景观的变化.根据艾比湖周边盐漠区盐尘的时空分布规律、活动特点和危害强度分析,盐尘对准噶尔盆地西部土壤盐分及景观变化的影响强度范围和影响程度划分为3级区.     

Trace Elements and Sr, Nd Isotope Geochemistry of the Lajimiao Norite-Gabbro from the North Qinling Belt

The Lajimiao norite-gabbro complex, as a part of the ophiolites on the southern side of the North Qinling belt, consists of gabbro and norite-gabbro. They were derived from different magma series: the gabbro was derived from tholeiitic magma series with higher TiO2, REE abundance and Fe3+/Fe2+ ratio ; norite-gabbro was derived from calc-alkali magma series with lower TiO2, Fe3+/Fe2+ ratio and REE abundance and much lower HREE abundance, which suggests that the source of the norite-gabbro magma was deeper and controlled by eclogite facies. Geochemical characteristics of both plutonic rocks are similar to those of island-arc basalts, such as relatively high contents of Ba, Pb and Sr and relatively low contents of Nb, Zr and N j.The Sr, Nd isotopic characteristics of the Lajimiao norite-gabbro complex are similar to those of ophiolites. Its εNd values are constant, about+2; whereas εst values have wide variation from - 6.4 to +31.2 and positively correlate with Na2O, H2O+ and CO2 contents and the Fe3+/Fe     

土水势、未冻水含量和温度

从热力学观点来看,土水体系中的水分迁移是由于该体系中的水处于不平衡状态引起的。这种不平衡状态是由许多力,包括物理、物理化学、力学和水分迁移期间产生的其它过程综合作用的结果。 除重力水之外,土中各种水都受到土矿物颗粒表面能的作用,或者说受到毛细力和吸附力的作用。     

Timing of Proterozoic magmatism in the Sunsas belt,Bolivian Precambrian Shield,SW Amazonian Craton

We present new U-Pb zircon and monazite ages from the Sunsas belt granitic magmatism in Bolivia,SW Amazonian Craton.The geochronological results revealed four major magmatic events recorded along the Sunsas belt domains.The older igneous event formed a granitic basement coeval to the Rio Apa Terrane(1.95-1.85 Ga)in the southern domain.The second magmatic episode is represented by 1.68 Ga granites associated to the Paraguá Terrane(1.69-1.66 Ga)in the northern domain.The 1.37-1.34 Ga granites related to San Ignacio orogeny represent the third and more pervasive magmatic event,recorded throughout the Sunsas belt.Moreover,magmatic ages of～1.42 Ga revealed that the granitogenesis asso-ciated to the Santa Helena orogeny also affected the Sunsas belt,indicating that it was not restricted to the Jauru Terrane.Lastly,the 1.10-1.04 Ga youngest magmatism was developed during the Sunsas oro-geny and represents the final magmatic evolution related to Rodinia assembly.Likewise,the 1.95-1.85 and 1.68 Ga inherited zircon cores obtained in the～1.3 Ga and 1.0 Ga granite samples suggest strong par-tial melting of the Paleoproterozoic sources.The 1079±14 Ma and 1018±6 Ma monazite crystallization ages can be correlated to the collisional tectono-thermal event of the Sunsas orogeny,associated to reac-tions of medium-to high-grade metamorphism.Thus,the Sunsas belt was built by heterogeneous 1.95-1.85 Ga and 1.68 Ga crustal fragments that were reworked at 1.37-1.34 Ga and 1.10-1.04 Ga related to orogenic collages.Furthermore,the 1.01 Ga monazite age suggests that granites previously dated by zir-con can bear evidence of a younger thermal history.Therefore,the geochronological evolution of the Sunsas belt may have been more complex than previously thought.     

http://www.sciencedirect.com/science/article/pii/S167498711100079X

Lower Paleozoic rocks exposed in various regions of Egypt (south central Sinai, north Eastern Desert and southwest Western Desert), in addition to occurring in the subsurface such as north Western Desert and the Gulf of Suez. The Lower Paleozoic rocks in Egypt include surface and subsurface rock units of formational status. The surface rock units are the Taba, Araba and Naqus formations. The subsurface rock units include the Shifa, Kohla and Basur formations. The Infracambrian Taba Formation has been discovered recently in the outcrops of the south eastern Sinai in the Taba-Ras El-Naqab area. It is missing and/or not recognized in the subsurface. The Taba Formation consists mainly of reddish brown, unfossiliferous gravelly fine-to medium-grained sandstones cemented by kaolinite and have subordinate beds of paleosols. The Cambrian Araba Formation and its subsurface equivalent (the Shifa Formation) are essentially composed of reddish brown, fine-grained laminated sandstone and siltstone with abundant Skolithos and Cruziana sp. In contrast, the Ordovician-Silurian Naqus Formation and its subsurface equivalents (Kohla Formation and Basur Formation) are mainly composed of white, unfossiliferous, cross-bedded, medium- to coarse-grained sandstones with haphazardly distributed pebbles and cobbles. Sedimentological analysis indicates that the Araba Formation and its equivalents were deposited in a marginal-marine environment, whereas the Naqus Formation and its equivalents were laid down in a fluvio-glacial environment. Integrated stratigraphic and sedimentological studies of the Lower Paleozoic rocks permit reconstruction of the paleogeography of Egypt at that time. Egypt has been largely controlled since the Cambrian by the pre-existing structural framework of the pre-Phanerozoic basement rocks inherited from the Late Proterozoic Pan-African event. Additionally, sedimentation processes were controlled during Cambro-Ordovician times by tectonic movements, whereas glacio-eustatic control predominated during the Late Ordovician-Silurian Period. These studies suggest that most areas of Egypt were exposed lands with episodically transgression by epicontinental seas related to the paleo-Tethys. These lands formed a part of a stable subsiding shelf at the northern Gondwana margin.     

澳大利亚与元三古代海底喷气矿床伴生的电气石岩

在绿片岩、角闪岩和麻粒岩和变质岩层中，电气石岩和富电气石的沉积物与喷气矿化伴生，它们遭受了中等到强烈的变形，呈连续层状分布于褶皱构造附近，显示出诸如层理、递变层理、交错层理、层内滑动等沉积构造和拉裂构造。在高级变质作用区，它们显示变质结构，通常被再活化而成的石英－电气石脉所穿切。富电气石岩出现在由海底喷气而形成的Pb－Zn－Ag、Cu－Co、Cu－Bi、W、Sn、Au和稀土元素矿化的下部、内部及矿化之上，且在横向上与矿化同期的地层中。在一些地方，电气石岩没有上述矿化现象，也不与花岗质岩石相伴生。电气石的成分是黑电气石－镁电气石，虽反映了其全岩成分，但不能作为矿化的标志。虽然电气石是与花岗岩、交代岩、角砾岩简伴生的普通矿物，但本文描述的富电气石层为山硅电气石前身的变质作用产生的富硼硅质铁建造。它们是一种常见的喷气岩类型，并且常常出现在早－中元古代厚层的泥质变沉积岩和蒸发岩层序中。这就说明硼是由含硼的粘土的淋滤作用或由含硼酸盐的蒸发岩的淋滤作用产生的。     

俄罗斯油气钻采废弃物处理及其利用研究

生态安全和环境保护是世界各国都非常关心的问题。地质钻探和石油天然气钻采工作中产生大量废弃物,直接影响生态安全和环境保护,给经济建设和人民生活带来很大的负面影响。俄罗斯钻探工作者对此进行了研究,取得了一定效果。他们主要采用综合处理方法和磁化处理方法。利用这2种方法,废弃物不仅可以再生,而且还可以二次使用,有一定的创新和实际意义,值得引起我们的重视,建议对此进行研究与讨论。     

热电离质谱法测定贵州郑家洞石笋的铀系年代及其古气候意义

本文报道了用高精度热电离质谱（ＴＩＭＳ）法测定的贵州郑家洞ＡＺＪ－２号石笋的铀系年代。该石笋经历了三个速度不同的生长阶段，顶部９０ｃｍ及底部２１ｃｍ生长迅速，ＴＩＭＳ铀系法高分辨率年代结果仍不足以给出其确切的生长速率。精确建立碳氧同位素演化时间坐标的困难，应是从新生碳酸盐提取古气候演变信息的重要制约因素之一。ＡＺＪ－２的生长起止年代为距今１４．７￣１３．８万年，贵州在此期间可能处于温暖湿润的气候条