多孔黏弹介质平面波理论及波场数值模拟

本文将黏弹固体骨架与各向异性多孔弹性模型相结合,并将地层黏弹性的特性考虑其中,更好地刻画了快P波和横波在地震频带的衰减现象。将多孔黏弹模型模拟结果同传统弹性模型模拟结果对比显示,多孔黏弹模型在模拟真实储层方面更具优势。     

基于定向片模型的SPOT-5遥感影像自检校光束法平差

本文通过建立内方位自检校模型,利用定向片模型对外方位元素进行内插建模,建立了基于定向片模型的自检校光束法平差,研究不同控制点数量和不同定向片间隔对定位精度的影响,并利用河南嵩山地区SPOT-5遥感影像数据对模型进行了实验验证和分析,结果表明,平面精度可以达到10.06m,高程精度可以达到8.84m.     

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)     

重磁等值线与经纬网的分离及其矢量化

本文利用经纬网在局部范围的直线性直线的平均ｆｒｅｅｍａｎ链码等于其上任意一点的链码的这一特性,达到自动分离经纬网与等值线的目的,为实现等值线图的自动矢量化打下了基础。     

沙漠地区风积沙地基输电线路装配式基础真型试验研究

沙漠风积沙地基输电线路杆塔基础设计是当前我国电网建设中的关键研究课题之一。沙漠风积沙属于特殊土地基,这种地基上的输电线路装配式基础缺少相关设计依据。针对沙漠风积沙地基输电线路基础工程的特点,进行了输电线路装配式基础的真型试验,得到了上拔与水平荷载、下压与水平荷载联合作用下的承载变形特性、基础构件的应变特性、基础底板与风积沙地基之间的接触压力变化规律。根据测试结果,确定了沙漠地区风积沙地基装配式基础的地基承载力和上拔角取值,得到了基础稳定的最不利工况,有助于提高基础设计的可靠性和合理性。试验结果为沙漠地区台远-塔中220 kV输电线路基础工程的设计提供了依据。     

华南飑线升尺度增长过程中的多尺度能量相互作用分析

采用WRF模式对华南飑线的升尺度增长过程进行模拟,利用Barnes滤波将模式数据分解为三个尺度,分别代入相应的能量方程中进行计算,从能量角度研究飑线升尺度增长过程中动能和位能的变化,以及三个尺度系统能量的相互转化。研究表明：动能的变化与飑线过程中各尺度系统的演变有较好的对应,β中小尺度对流的发展对应β中小尺度系统动能的变化,而在飑线升尺度增长过程中,α中尺度系统动能快速增长。在飑线发展过程中环境场通过位能向动能的转化使得β中小尺度对流快速发展加强,而β中尺度飑线的快速发展与合并加强导致了飑线的升尺度增长。在飑线的升尺度增长过程中,β中小尺度动能大量转化为α中尺度动能使得α中尺度飑线迅速增强,而环境场对飑线升尺度增长过程的直接影响较小。     

甘肃玛曲大水金矿田控矿因素及主矿体特征对比分析

大水金矿田由大水、贡北、格尔托3处大、中型金矿床组成,经过30年巨量探矿工程的投入和持续有效的勘查与研究,整体达到了详查程度,累计查明金资源量约130 t,为典型矿床对比研究提供了理想基地。通过大水金矿田赋矿地层岩性、控矿断裂构造、成矿侵入岩等控矿因素的对比分析认为：大水金矿田赋矿地层岩性以中三叠统马热松多组灰岩为主;控矿断裂、成矿容矿脉岩及其所赋存矿体的规模,以大水特大型金矿明显优于贡北、格尔托中型金矿,大水金矿主要以NWW向压扭性主干断裂与近SN向放射状张性断裂的交汇部位控制厚富主矿体,贡北以EW向、格尔托以NNW与NE向断裂的交汇部位控制主矿体的分布;中酸性岩体及其派生的酸性岩脉与金成矿关系密切,容矿花岗闪长岩（斑）岩脉及其蚀变方解石大脉在陡倾断裂破碎带中的集中分布,往往指示厚富金矿体的赋存地段。通过3个矿区主矿体的规模、品位、资源量分布等特征的对比分析可以看出,主矿体的规模、品位以大水较贡北、格尔托为大、为富,大水、贡北、格尔托金矿的主矿体资源量分别占矿区的75. 62%、78. 51%和79. 58%,且由普查到详查,主矿体资源量占比有所变化,如大水金矿由70. 59%增加到75. 63%,贡北金矿则由88. 24%降低为84. 16%。     

DCMT光电扫描主测微器的设计与研究

DCMT主测微器不同于其它类型的子午环测微器,它具有自校准测定仪器参数的功能。该测微器采用了活动光栅的方案,其优点是能观测近极星和各类准直像;活动光栅另一个显著优点是不同赤纬星几乎可用相同的观测时间.对“V”形光栅的工作原理和误差进行了详细讨论,并给出了一组严格的公式。其系统误差来源有:光栅形状改正、光栅驱动方向相对于光栅的倾斜、光栅驱动方向相对于赤径方向的倾斜、星径曲率改正。     

Stratigraphic architecture and sedimentology of a Late Pleistocene subaqueous moraine complex,southwest Ireland

Glacigenic sediments exposed in coastal cliffs cut through undulatory terrain fronting the Last Glacial Maximum laterofrontal moraine at Waterville on the Iveragh Peninsula, southwest Ireland, comprise three lithofacies. Lithofacies 1 and 2 consist of interdigitated, offlapping and superimposed ice‐proximal subaqueous outwash and stacked sequences of cohesionless and cohesive subaqueous debris flows, winnowed lag gravels and coarse‐grained suspension deposits. These are indicative of sedimentation in and around small grounding line fans that prograded from an oscillating glacier margin into a proglacial, interlobate lake. Lithofacies 3 comprises braided river deposits that have undergone significant syn‐sedimentary soft‐sediment deformation. Deposition was likely related to proglacial outwash activity and records the reduction of accommodation space for subaqueous sedimentation, either through the lowering of proglacial water levels or due to basin infilling. The stratigraphic architecture and sedimentology of the moraine at Waterville highlight the role of ice‐marginal depositional processes in the construction of morphostratigraphically significant ‘end moraine’ complexes in Great Britain and Ireland. Traditional ‘tills’ in these moraines are often crudely stratified diamictons and gravelly clinoforms deposited in ice‐proximal subaqueous and subaerial fans. Copyright © 2011 John Wiley & Sons, Ltd.