河北东坪金矿区水泉沟岩体的地球化学特征

水泉沟岩体主要由二长岩构成。主要矿物是碱性长石和斜长石,它们的含量高达80%以上。石英不多见,暗色矿物含量少。副矿物主要是磁铁矿、石榴石、榍石和锆石。交代结构发育,蚀变现象普遍。主要化学组分和微量元素含量及δ¹⁸O值变化范围大。该二长岩体是由老片麻岩经热液碱交代作用而成。     

内蒙古白银都西群变质火山岩的钕、锶同位素研究

白银都西群主要由斜长角闪岩、变粒岩、长英片岩和条带状混合岩组成,是白银都西-白乃庙地体的重要组成部分,主要分布在内蒙古白乃庙铜(金)矿床东北白银都西一带。长期以来,由于缺乏可信的同位素年龄数据,该套岩层的归属,构造性质和形成机理尚不清楚。笔者首次对白银都西群斜长角闪岩的Nd和Sr同位素组成进行了测定,所获Sm-Nd同位素等时年龄为1394±46Ma(23),Nd初始比值为0.511 243±8(23)和εNd(T)=+7.9±2.1(23)。~(87)Sr/~(86)Sr和~(87)Rb/~(86)Sr比值分别为0.705 79—0.709 12和0.17—0.34,两者之间不存在任何相关关系。结合野外地质证据和岩相学特征,我们认为:白银都西群基性火山活动发生在中元古代,成岩物质来自亏损地幔源,成岩以后构造变动和变质热液活动致使Rb-Sr同位素体系受到严重干扰破坏。     

福建上杭盆地中生代火山岩首次发现开来石

在１：５万上杭幅重砂野外调查中，在上杭盆地中生代火山岩河系中首次发现开来石。经中国地质大学Ｘ光单晶粉晶分析、桂林有色金属地质研究所电子探针成分分析结果，均与国外有关文献中的开来石相一致。是我省首次发现的含砷稀土矿物。它为在该区中生代火山岩中寻找稀土资源提供新的线索。此外该矿物常与黄金、辰砂等相伴生，笔者初步认为可以根据伴生金的相关元素Ａｓ开来石组合寻找金，是本区很值得注意的一种寻找金的方法。     

福建浦城丘源地区晚太古代变质岩地质特征

浦城丘源地区出露太古代变质岩，其地质特征类似于建宁西部上太古界天井坪组，并取得了２６７８±４１Ｍａ同位素年龄资料。本文系统论述其岩石组合、原岩建造、大地构造环境及同位素地质年龄等特征。     

北京密怀平山区金矿成矿地质条件及成矿期的探讨

本文通过对密怀平山区金矿成矿地质条件的分析，将密怀平山区金矿的成矿期划分为早元古代吕梁成矿期、中生界印支成矿期及燕山成矿期三个成矿期。     

闽粤台沿海北西西向最新构造带与大震构造背景

闽粤台沿海自台湾运动以来逐渐形成了多条北西西向隆起—拗陷的最新活动构造带,与已知的北东—北北东向隆起、拗陷带构成了区域性镶嵌构造格局。 研究区内除板块相互碰撞、俯冲及上地幔物质上涌形成大震构造背景外,莫霍面隆起或隆起断距大、低速层厚、地壳变薄、近两、三千年地表抬升差异活动显著以及台东近海有北西西向构造活动等,也都是发生大震的重要构造背景     

Study of the crust and mantle using magnetic surveys by Magsat and other satellites

Among the first measurements made from near-Earth orbiting satellites were measurements of the magnetic field. The sources of that field lie both within the Earth, in its core and crust, and in the surrounding ionosphere and magnetosphere. This article summarizes some of the methodology and results for studies of the Earth’s mantle and crust. Mantle conductivity studies can be made either by studying signals impressed on the Earth from outside, e.g., the ionosphere or magnetosphere, or by studying signals originating in the core and transmitted through the mantle. Crustal field studies begin with a careful selection of the data and subsequent removal of core and external fields by some sort of filtering. Average maps from different local times sometimes differ, presumably due to the remaining presence of fields of external origin. Several techniques for further filtering are discussed. Where large-area aeromagnetic maps are available, crustal maps derived from satellite data can be compared with upward continued data. In general, the comparisons show agreement, with some differences, particularly in and near the auroral belts. The satellite data are further reduced by various methods of inverse and forward modelling, sometimes including reduction to the pole (RTP). These techniques are generally unstable at the equator. Common methods of stabilizing the inversions include principle components analysis and ridge regression. Because of the presence of the core field, the entire crustal contribution from the field is not known. Also, there is a basic nonuniqueness to the inverse solutions. Nevertheless, magnetizations that are interpretable can be derived.     

Palaeomagnetism and rock magnetism of the Deccan traps

Extensive work on the palaeomagnetism of the Deccan traps by several workers has revealed only one reversal (normal-reverse-normal) of the geomagnetic field during the period of eruption of these flows. The scatter in the natural remanent magnetic directions of different flows in a sequence of these traps is rather large and it persists even after magnetic cleaning. Generally this large scatter of directions is attributed to the geomagnetic secular variation during formation of the traps. Recent studies of the magnetic properties of the trap samples indicate that the presence of multidomain magnetite in a lava sequence differs from locality to locality in the Deccan trap province and so the stability of their natural remanent magnetization. While these features can be clearly perceived, an understanding of the same seems to be quite difficult. However, it appears that part of the scatter in directions could be due to the alteration of the magnetic minerals in the Deccan traps and hence it would not be proper to relate the entire scatter to the secular variation.