扬子北缘奥陶纪—志留纪之交泥岩地球化学特征及其源区、构造背景

近年来,扬子地块北缘奥陶纪—志留纪之交沉积构造背景一直存在不同认识。本文对渝东北城口厚坪五峰组—龙马溪组砂、泥岩进行系统采样和主、微量元素测试分析,从地球化学特征角度,来探讨该时期砂、泥岩物源源区及其构造环境。地球化学特征显示,五峰组—龙马溪组砂、泥岩主量元素SiO2含量为39.57%～87.16%,多数高于北美页岩,Al2O3含量为3.41%～14.98%,均低于北美页岩,MgO、CaO、MnO2和P2O5含量明显低于北美页岩,相比于四川盆地川南长宁—双河五峰组—龙马溪组泥岩,渝东北城口具有高SiO2和低MgO、CaO的特点,表明城口五峰组—龙马溪组泥岩碎屑组分主要以粉砂质和硅质等陆缘碎屑为主;微量元素Sc、Sr、Co、Zr、Hf较北美页岩相对亏损,V、U、Sb、Ba相对富集,Cr、Ni、Nb、Ta含量相近。稀土元素北美页岩标准化均表现为略微向右倾斜的配分模式,多数具有δCe负异常,观音桥段和龙马溪组δEu正异常指示了该时期存在海底热液活动。砂、泥岩主、微量元素的物源和构造背景图解表明沉积物源区源岩具有多样的物质组分,以长英质岩为主,同时混入了花岗质和安山质岩石组分;源岩形成时的构造背景主要为被动陆缘环境,少数为活动陆缘和大陆岛弧环境,这一结果与扬子地块北缘新元古代—早古生代处于被动大陆边缘的区域地质背景一致。     

滑坡体多排列电阻率联合成像探查试验研究

正滑坡是自然界最为普遍的地质灾害,尤其随着工程建设的高速发展,新建工程设施诱发的滑坡现象时有发生,进而产生一系列经济和社会问题。为减少滑坡造成的损失,采用有效的技术手段查明滑动面的空间位置是实施灾害治理的前提和关键。在地质勘察中,钻探能直观的揭露出不同深度岩土体的分布特征及物理力学参数,从而有效的推断出滑动软弱带的信息,但实际应用中滑坡带的范围较大,离散化的钻孔资料显然存在信息量不足的弊端,并且随机布局的钻孔并也不能提供最科学的地质信息。     

南海东北部陆坡天然气水合物区的滑塌和泥火山活动

本文研究了南海东北部陆坡天然气水合物区滑塌和泥火山活动的特征及表现形式,探讨了滑塌和泥火山活动对天然气水合物成藏的影响,提出了滑塌主导和滑塌、泥火山共同作用两种控制模式。根据地震数据、浅层剖面和海底地形数据解释,将研究区划分为规则滑塌区和泥火山活动影响区,并识别出泥火山、泥火山脊、凹槽、凹坑等特征地形。滑塌和泥火山活动是陆坡天然气水合物发育区重要的地形控制因素,两种活动共同作用产生复杂的地形特征。综合多条地震测线中似海底反射层(BSR)形态、连续性和滑塌、泥火山活动的关系,认为滑塌控制的区域,BSR连续,天然气水合物储藏较完整,泥火山活动区天然气水合物储藏也仅受到局部破坏。同时指出滑塌和泥火山活动对研究区长期天然气渗漏活动具有重要作用。     

Exploring the Moon's surface for remnants of the lunar mantle 1. Dunite xenoliths in mare basalts. A crustal or mantle origin?

Remotely sensed observations from recent missions (e.g., GRAIL, Kaguya, Chandrayaan‐1) have been interpreted as indicating that the deep crust and upper mantle are close to or at the lunar surface in many large impact basins (e.g., Crisium, Apollo, Moscoviense). If this is correct, the capability of either impact or volcanic processes to transport mantle lithologies to the lunar surface should be enhanced in these regions. Somewhat problematic to these observations and interpretations is that examples of mantle lithologies in the lunar sample collection (Apollo Program, Luna Program, lunar meteorites) are at best ambiguous. Dunite xenoliths in high‐Ti mare basalt 74275 are one of these ambiguous examples. In this high‐Ti mare basalt, olivine occurs in three generations: olivine associated with dunite xenoliths, olivine megacrysts, and olivine microphenocrysts. The dunite xenoliths are anhedral in shape and are generally greater than 800 μm in diameter. The interior of the xenoliths are fairly homogeneous with regard to many divalent cations. For example, the Mg# (Mg/Mg + Fe × 100) ranges from 82 to 83 in their interiors and decreases from 82 to 68 over the 10–30 μm wide outer rim. Titanium and phosphorus X‐ray maps of the xenolith illustrate that these slow diffusing elements preserve primary cumulate zoning textures. These textures indicate that the xenoliths consist of many individual olivine grains approximately 150–200 μm in diameter with low Ti, Al, and P cores. These highly incompatible elements are enriched in the outer Fe‐rich rims of the xenoliths and slightly enriched in the rims of the individual olivine grains. Highly compatible elements in olivine such as Ni exhibit a decrease in the rim surrounding the xenolith, an increase in the incompatible element depleted cores of the individual olivine grains, and a slight decrease in the “interior rims” of the individual olivine grains. Inferred melt composition, liquid lines of descent, and zoning profiles enable the reconstruction of the petrogenesis of the dunite xenoliths. Preservation of primary magmatic zoning (Ti, P, Al) and lack of textures similar to high‐pressure mineral assemblages exhibited by the Mg‐suite (Shearer et al. 2015) indicate that these xenoliths do not represent deep crustal or shallow mantle lithologies. Further, they are chemically and mineralogically distinct from Mg‐suite dunites identified from the Apollo 17 site. More likely, they represent olivine cumulates that crystallized from a low‐Ti mare basalt at intermediate to shallow crustal levels. The parent basalt to the dunite xenolith lithology was more primitive than low‐Ti basalts thus far returned from the Moon. Furthermore, this parental magma and its more evolved daughter magmas are not represented in the basalt sample suite returned from the Taurus‐Littrow Valley by the Apollo 17 mission. The dunite xenolith records several episodes of crystallization and re‐equilibration. During the last episode of re‐equilibration, the dunite cumulate was sampled by the 74275 high‐Ti basalt and transported over a period of 30–70 days to the lunar surface.     

在空间数据库课程中采用开源软件实验的教学实践

对比分析了国内外空间数据库课程现状。针对开源地理空间信息软件体系在空间数据库实验课程中的教学特点,探讨了开源软件应用于空间数据库课程实验的教学实践,提出了分阶段实验教学方法,在实际教学中取得了好的效果。     

新疆天文台25m VLBI、GPS归心测量

介绍了2011年中国科学院新疆天文台南山站GPS和25m VLBI天线的归心测量方案、局域三角测量网、高程控制网与靶标交会测量方法及资料解算。利用测量数据,首次建立了南山GPS与VLBI空间大地测量技术并置站本地连接参数,测量精度优于1mm。     

GNSS 系统中新 BOC信号性能评估研究

卫星信号体制是卫星导航系统性能的决定性因素之一,无论是BDS 或Galileo等新系统的建设还是GPS或GLONASS等系统的现代化过程中,导航信号的设计与性能评估都是所关注的焦点,BOC调制是GNSS的重要选择,本文引入一种GNSS中有效可调带宽的信号波形以减轻多径和干扰的影响。仿真结果表明：该波形在精度、多径抑制和抗干扰方面较普通BOC具有更好的性能。     

Understanding Today's Online GIS User Through the Lens of a WorldMap Survey

WorldMap is an open source online mapping application which aims to lower barriers for scholars who wish to visualize, analyze, organize, present, and publish mapped information. In late 2013, 290 respondents among the 8,000 registered users participated in an online survey in which they described their activities, purposes, experiences, and preferences regarding the system. Participants also described their professional background, GIS skill level, age, gender, and country of work. This study analyzes the results of the survey, by summarizing the responses to each question independently and by examining the relationships and dependencies of these answers across the different questions to try to better understand why users responded the way they did. The study is based on the user‐centered design (UCD) approach. We aim to use the survey results to improve our understanding of user demographics and needs. Findings from this study will be used to guide WorldMap improvements, and we hope the findings will also shed light on the broader requirements of online GIS users.     

地球外部扰动重力严密改化模型及分析检验

直接积分模型是计算地球外部扰动重力的主要数学工具,将全球积分模型改化为局域积分模型是实现地球外部重力场赋值的前提条件.相比表层积分模型和向上延拓积分模型,Stokes积分模型要求的输入信息种类最少,故在减轻数据保障压力方面具有比较明显的优势.在实施Stokes积分模型工程化应用过程中,我们发现扰动重力径向分量积分模型从...     

中国磷矿资源预测模型及找矿远景分析

[研究目的]磷矿是具有战略意义的矿产资源,2014年至今,中国地质调查局组织编写的中国矿产地质志,全面描述了中国磷矿全貌及重要成矿规律,加强了对全国磷矿矿情的掌握.本文依托中国矿产地质志项目,系统总结了中国磷矿时空分布特征,圈定了磷矿找矿远景区和磷矿重点勘查区,对未来磷矿找矿工作有一定的参考价值.[研究方法]本文选取了...