The significance of rock structure,lithology and pre‐glacial deep weathering for the shape of intermediate‐scale glacial erosional landforms

The main landforms within the glacially scoured Precambrian rocks of the Swedish west coast are closely connected to the principal structural pattern and have lately been explained as mainly a result of etch processes, probably during the Mesozoic and with a possible second period of etching during the Neogene. To explore the effect of multiple glacial erosion on the rock surfaces, an island with two different lithologies and with striae from different directions was selected for a detailed study, focusing on the shape of roches moutonnées. Air‐photo interpretation of bedrock lineaments and roches moutonnées combined with detailed field mapping and striae measurements are used to interpret the structural and lithological control on the resulting shape. The study reveals a significant difference in shape between roches moutonnées in augen‐granite and orthogneiss. Low elongated and streamlined roches moutonnées occur in the gneiss area, striated by a Late Weichselian ice flow from the NE. This ice flow is subparallel with both the local dominant trend of topographically well‐expressed joints and the schistosity of the gneiss. Frequently, there are no signs of quarrying on the lee‐sides of the gneiss roches moutonnées and hence they resemble the shape of whalebacks, or ruwares, as typically associated with the exposed basal weathering surface found in tropical areas. The granite roches moutonnées were formed by an older ice flow from the ESE, which closely followed the etched WNW–ESE joint system of the granite. Late Weichselian ice flow from the NE caused only minor changes of the landforms. On the contrary, marks of the early ESE ice flow are poorly preserved in the gneiss area, where it probably never had any large effect as the flow was perpendicular to both schistosity and structures and, accordingly, also to the pre‐glacial relief. The study demonstrates that coincidence between ice flow direction and pre‐glacially etched structures is most likely to determine the effects of glacial erosion. Copyright © 2002 John Wiley & Sons, Ltd.     

武汉基准台超导重力仪重力潮汐观测结果

本文采用重力残差信号对武汉基准台超导重力仪的原始观测数据（２０秒采样）作预处理，将原始观测信号分解成重力潮汐和残差两部分，在残差信号中消除一些已知的干扰因素的影响。利用ＥＴＥＲＮＡ软件作调和分析，两主波（Ｏ１和Ｍ２）的重力潮汐参数（振幅因子和相位滞后）为：Ｏ１：１．１７８８±０．０００６，－０．５９７５°±０．０２８°；Ｍ２：１．１７１３±０．０００２，－０．５８７３°±０．００８°经海潮改正以后，Ｏ１和Ｍ２波的潮汐参数与Ｗａｈｒ－Ｄｅｈａｎｔ潮汐模型值相比，振幅因子的偏差优于０．１％。     

集合预报及其在中期天气预报中的应用

作者概述了集合预报的基本概念，集合预报中期天气预报中的意义与作用，现有的主要集合预报产品以及集合预报在美国美国国家气象中心和欧洲中期天气预报的业务运行。简要介绍了我国国家气象中心在动力延伸预报和集合预报方面的试验研究情况。     

滇西西盟地区前泥盆纪变质岩系的变形构造格架

滇西西盟一带是保山—掸邦地块在我国境内的一个基底岩系出露地区。该地区的前泥盆纪变质岩系可划分成两个构造层，下部为元古代构造层，由变质深度达角闪岩相的怕可杂岩系组成，发育３期南北向的变形构造；上部为早古生代构造层，由低绿片岩相变质的王雅组、允沟组组成，发育两期呈南北向的变形构造。变形构造表明，西盟变质岩系的主期构造格架以怕可—老街子背形叠瓦垛为主导构造要素，由背驮式扩展的向东逆冲的盲逆冲断裂系组成，王雅—允沟反冲叠瓦扇是盲逆冲断裂系的盖层响应变形系统，并以向西逆冲的推覆构造为特征     

广西前汛期旱涝特征及成因分析

利用 EOF分解和 Z指数对广西前汛期 (4～ 6月 )降水进行型态分布及旱涝等级的划分 ,研究旱涝的空间分布、年际变化及年代际变化 ,并对旱涝成因进行了分析。结果表明 :广西前汛期降水的一致性较好 ;6 0年代和 90年代为旱涝多发年代 ,70年代以涝为主要特征 ,80年代以旱为主要特征。影响广西前汛期降水的环流因子主要有中高纬环流经向度、北半球极涡、印缅槽及副热带高压 ;中低纬太平洋海区对广西前汛期降水多少的影响亦较明显     

数字式智能化锚索预应力传感器的研究与设计

预应力传感器是锚固工程，预应力混凝土工程，预应力桥梁工程等领域进行监测，研究与试验必不可少的测量用传感器，在分析预应力传感器[研究现状的基础上，详细了介绍了数字式智能化锚索预应力传感器的工作原理，结论设计，计量检定结果，主要特点和应用情况。     

钻头预合金胎体粉末制备与应用

讨论了预合台体粉末的优点，研究了预合金胎的粉末的制备技术，列举了预合金胎体金刚石钻头的应用效果。     

南昆铁路新型、轻型支挡结构的设计与施工

介绍了南昆铁路应用的各种新型,轻型支档结构及其设计与施工经验,并论述了适用条件。     

Gas emission prediction and recovery in underground coal mines

Strata gas can be released and captured from non-active and active gas resources either from virgin or relaxed strata, both prior to and when mining activities take place. The high and irregular gas emissions associated with high production longwall mining have provided a need to optimise the methods used to predict these gas levels and the ventilation requirements for gas dilution. A forecast of gas emissions during development drivage and longwall mining indicated possible gas and ventilation problems requiring the introduction of various gas drainage techniques and in maintaining the necessary air quantities in ventilation systems to satisfy the statutory gas limitations for various coal production rates. Although there are sound principles used in world-recognised methods of gas emission prediction, a new approach developed from long-term practical experience in underground gassy coal mine practices and gas-rock mechanics studies appear most suitable for local conditions and mining systems in use. The Lunagas ‘Floorgas' and ‘Roofgas' geomechanical and gas emission models offer an effective solution to these problems. Both programs are the most advanced engineering, numerical tools available to calculate gas source contributions to total gassiness and improve the accuracy and quality of gas control, gas capture technologies and ventilation system design.     

Chemical spots on the surface of the strongly magnetic Herbig Ae star HD 101412

Due to the knowledge of the rotation period and the presence of a rather strong surface magnetic field, the sharp‐lined young Herbig Ae star HD 101412 with a rotation period of 42 d has become one of the most well‐studied targets among the Herbig Ae stars. High‐resolution HARPS polarimetric spectra of HD 101412 were recently obtained on seven different epochs. Our study of the spectral variability over the part of the rotation cycle covered by HARPS observations reveals that the line profiles of the elements Mg, Si, Ca, Ti, Cr, Mn, Fe, and Sr are clearly variable while He exhibits variability that is opposite to the behaviour of the other elements studied. Since classical Ap stars usually show a relationship between the magnetic field geometry and the distribution of element spots, we used in our magnetic field measurements different line samples belonging to the three elements with the most numerous spectral lines, Ti, Cr, and Fe. Over the time interval covered by the available spectra, the longitudinal magnetic field changes sign from negative to positive polarity. The distribution of field values obtained using Ti, Cr, and Fe lines is, however, completely different compared to the magnetic field values determined in previous low‐resolution FORS 2 measurements, where hydrogen Balmer lines are the main contributors to the magnetic field measurements, indicating the presence of concentration of the studied iron‐peak elements in the region of the magnetic equator. Further, we discuss the potential role of contamination by the surrounding warm circumstellar matter in the appearance of Zeeman features obtained using Ti lines. (© 2016 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)