拉尔玛硅岩型金—铜—铀建造矿床的海底喷流沉积特征及找矿方向

西秦岭南亚带中的拉尔玛硅岩型金-铜-铀矿床,是一个比较典型的与海底喷流作用有关的金矿床。矿床赋存于寒武系太阳顶群中。太阳顶群地层由硅岩、板岩组成,厚度近千米。现已发现的矿体,80％以上产于硅岩中。硅质岩的地质地球化学特征表明,它是海底喷气沉积作用的产物,拉尔玛金-铜-铀建造矿床也具有海底喷流的沉积特征。     

小莱河麻粒岩相铁建造的矿物组合—变质过程p、T变化的探讨

小莱河太古宙麻粒岩相铁建造的矿物组合有：①斜方辉石（Fs87）＋钙铁辉石＋石英＋磁铁矿±莱河矿；②铁闪石＋铁浅闪石质角闪石＋石英＋磁铁矿＋碳酸盐±Fe－镁川石（云辉闪石）。辉石的出溶显示了它形成的不同阶段：片晶发育的OpxⅡ－CpxⅡ是最后稳定产物，计算的平衡温度是742℃，按相图获得的压力是7×108～7．8×108Pa；钙铁辉石中“001”片晶是易变辉石片晶转变的，Opx－Cpx－Pig（片晶）阶段据相图推测可能形成于近820℃，8×108Pa的条件下。原始均一相的OpxⅠ－CpxⅠ阶段矿物成分按估算的片晶含量计算，它们的形成温度接近820℃，可能的压力范围是11×108～13×108Pa。由此得到ITD型麻粒岩相p－T－t轨迹。莱河矿无氧化成因的证据，认为它是在麻粒岩相条件下生成的。云辉闪石的Si—O链重复周期是3×，其Fe／（Fe＋Mg）＝0．85，是接近富铁端元的Fe－镁川石，它与闪石一起在640到近700℃条件下交代了辉石。     

四扣地区高精度目标地震采集技术研究

在四扣地区，由于地下地质构造非常复杂，老观测系统炮检距分布不均，方位角较窄，覆盖次数较低，使义东大断裂系统及潜山构造的资料信噪比较低，无法进行精细的构造解释和油藏描述。为了得到该目标区域的资料，作者在文中提供了一种解决思路，即针对复杂地质构造进行精细的目标地震采集设计，并在野外实际生产中运用了一系列的高精度采集技术手段和措施，使目标区域内的资料整体水平比以往有了较大幅度的提高，最终可获得用于精细构造解释的地震剖面。从本次采集在该地区成功应用的实例表明，目标地震采集技术对于解决复杂地质构造区域资料较差的问题是一种很好的方法，对以后类似工区的采集具有参考价值。     

应用气压、暴雨标定地下水位的应力格值及其意义

随着地下水动态观测工作的开展以及观测仪器的改进,在不少井孔的观测中,观测到了由气压变化、急剧降水引起地下水位的变化现象。此现象一般称为“气压效应”和“暴雨效应”。笔者认为,研究气压效应及暴雨效应有更广泛的意义。例如,应用气压效应及暴雨效应来确定井孔地下水位的应力格值将有助于对井孔地下水位的基本特征的认识,有     

北京北苑居住区第四系断层走向勘察

介绍了北京北苑居住区第四系断层走向勘察的工作方法,提出了在平原地区进行岩土工程勘察时应注意发现地层在水平方向变化的问题,并根据区域性的地层对比划分两个工程地质区,用剖面追索法准确确定分区界线,并论证了该界线的形成与黄庄—高丽营隐伏断层的第四纪继承性活动有关     

利用相关分析划分重力异常

本文从理论上对相关分析法区分重力异常的可行性进行了论述，并从一元线性回归方程着手，对大地水准面上的重力值与相应的地形高程作了相关分析，通过分析，认为在区域性小比例主均衡补偿基本完善的条件下，重力值与高程有极好的线性相关关系；当计算窗口较大时，地下的局部不均匀体，不足以破坏重力值与高程的相头发一，所以，在实际工作中，利用相关分析处理重力资料的叠加场，可以收到较好的效果，且方法简单易行。     

Primordial non-Gaussianity from LAMOST surveys

The primordial non-Gaussianity (PNG) in the matter density perturbation is a very powerful probe of the physics of the very early Universe. The local PNG can induce a distinct scale-dependent bias on the large scale structure distribution of galaxies and quasars, which could be used for constraining it. We study the detection limits of PNG from the surveys of the LAMOST telescope. The cases of the main galaxy survey, the luminous red galaxy (LRG) survey, and the quasar survey of dif- ferent magnitude limits...     

Research on Paleoecology of Middle Permian-Middle Triassic in the Western Sichuan Basin

The research area is located in the western part of Sichuan basin as a Yangtze ecotope of Cathaysian Tethyan area. It is dominated by benthic fauna, including brachiopods, Fusulinids, corals, bivalves, foraminifers, ammonites, bryozoans,Crinoids and pleopods which are less common with traces of trilobites, stromatoporas, nautilus and sporopollens seen in one or two areas,which are obviously controlled by sedimentary environments and in accordance with sedimentary facies.Through the analysis of fossils and research on burial characteristics from middle Permian middleTriassic, based on the combination of the feature of fossils in time and space, seventeen communities are recognized, the coposition, construction and palaeoenvironment of each community are expounded. Study shows that different ecological type biocoenose are distributed in different locations, which are mainly represented by sessile benthic community in the main research area, composed of Mianzhu, Mianyang, Deyang and Santai and nektonic community in marginal areas in the research area subdivided into two parts: Areas around Guangyuan-Nanjiang-Tongjiang, located at the margins in the northeast of the research area, and areas around Wenchuan-Maoxian-Dayidafeishui situated at the western borders of the research area. According to the combination of communities with sedimentary characteristics,six kinds of biofacies have been recognized and described in the study area and biofacies pattern are established. Category,ecotype, typical community and sedimentary facies of each biofacies are elucidated in this paper. The subdivision and analysis of community are meaningful for the studies of paleoenvironment ,paleogeography and their evolutions,The research of biaofacies is important for the recovery of paleobiogeography and paleoplate tectonic characteristics.     

基于走航观测数据的ERA5南海北部夏季短波辐射收支评估

海表短波辐射收支是海–气界面能量交换的重要物理过程。本研究利用2019年南海北部夏季科考航次的走航观测数据,评估了ERA5再分析数据的海表短波辐射通量收支。结果表明,ERA5的向下短波辐射相比观测偏小,11时和15时（北京时间）的偏差最大,可达−100 W/m² 。与此同时,ERA5的海表反照率整体偏低,其中高太阳高度角时段偏差较小,约为−0.03,低太阳高度角时段偏差较大,约为−0.15。向下短波辐射和反照率的偏差共同造成ERA5白天平均海表净短波辐射通量比观测偏小约25.4 W/m²;其中,反照率低估抵消了约50%向下短波辐射偏差的贡献。研究表明,在不同大气透射率情况下,ERA5的海表辐射收支偏差存在不同表现。ERA5海表反照率的低估可能与其采用的参数化方案在南海北部的适用性不足有关。基于观测本研究也给出了一个简单的参数优化方案。