康西瓦南岔路口地区早石炭世地层化石的发现

本次区调在1:25万岔路口幅向阳峰一带地质填图和实测地层剖面中,在原划中泥盆统落石沟组中采到了大量腕足、珊瑚类化石,经鉴定其形成时代为早石炭世中期.该套地层与西邻<神仙湾>幅区域地层对比,厘定为早石炭世帕斯群.该生物化石的取得,为该套地层时代划分提供了依据,填补了岔路口地区缺失早石炭世地层的空白,为进一步详细研究甜水海微陆块地层层序格架及地层演化,提供了新的基础资料.     

三峡工程库区迁建城镇新址地质环境质量综合评价与对比

通过建立地质环境质量综合评价指标体系,运用灰色聚类方法,对三峡工程库区九座迁建城镇新址的地质环境质量进行了综合对比分析,划分出三个质量等级。地质环境质量等级反映了迁建城址环境组成要素与人类工程活动和社会经济发展的适宜程度。单要素地质体质量,城市综合灾度和自然资源优势度是主要的影响因素。     

中国海洋产业发展的地区差距变动及空间集聚分析

采用基尼系数、变异系数、加权变异系数等指标,分析了20世纪90年代海洋经济发展的地区差距以及海洋产业空间集聚的变动趋势。得出以下结论,90年代前半期,我国海洋经济的相对地区差距缩小,后半期有所扩大。90年代多种海洋产业在同一地区的空间集聚减弱。其中,1995年到2000年多种海洋产业的空间集聚加剧。我国海洋经济地区差异与多种海洋产业的同一空间集聚表现为相同的变动过程。     

基于地理杂志阅读与手机软件应用的地理假期作业实施与反思

许多高中生的假期是用来打“题海战役”的,面对海量的作业学生很难提起精神,能认真完成作业的学生少之又少。设计怎样的假期作业既能吸引学生又能提高学生地理核心素养是教师需要做的功课。笔者借助杂志与手机软件设计了两项地理假期作业,以供同行探讨。     

基于网格细分技术的三维地质模型光滑方法研究

针对粗糙的三维地质模型,利用网格细分技术,生成加密光滑的三维模型。分析网格细分技术在三维地质建模中的应用需求以及Loop细分和改进的蝶形细分技术,为保持地质体之间公共面数据的一致性,对"改进的蝶形细分法"做了进一步改进,增加了对边界约束的处理。探讨利用细分技术生成多分辨率模型,通过试验验证了该方法的有效性。     

湖南保靖县且溪科铅锌矿地质特征

且溪科铅锌矿位于湖南省保靖县。区内倒转褶皱和断裂构造彼此贯通,形成良好的导矿构造系统,对区内铅锌矿的控制最为明显。铅锌矿体呈似层状形态大致顺层产于寒武系下统清虚洞组灰色中层夹薄层条带状粉—细晶云岩、砾屑白云岩和层间碎裂岩、角砾岩内。矿区铅锌矿床的形成是区域构造、矿区地质构造、沉积建造、热液活动等多种地质作用的综合产物,其中矿区地层岩性与岩相、构造是本矿床成矿控制的主要因素。位于麻栗场断层上盘褶皱构造内的寒武系下统清虚洞组上段白云岩,是该区铅锌矿的主要找矿方向,有希望找到大中型铅锌矿床。     

The dynamo theory of plasma turbulence wave in rotating celestial bodies

The various modes of plasma turbulence waves (including MHD waves) are easily excited under cosmic circumstances. In this paper, if we consider that the celestial bodies rotate, there is a source term generated for the magnetic induced equation by the excited plasma turbulence waves. If we expand the turbulent field in the Fourier series and include rotation velocity, the dynamo equation for turbulent waves is obtained. We have also obtained the solutions of various wave forms corresponding to different rotation velocities and then we significantly discuss the magnetic fields in the Sun, planets, and other celestial bodies.     

The JVAS/CLASS search for 6-arcsec to 15-arcsec image separation lensing

The Jodrell Bank–VLA Astrometric Survey (JVAS) and the Cosmic Lens All Sky Survey (CLASS) have been systematically searched for multiple gravitational imaging of sources with image separations between 6 arcsec and 15 arcsec, associated with galaxy group and cluster lensing masses. The radio and optical follow-up observations of all candidates are presented. From a total of ∼15 000 sources only one weak candidate remains and this is not contained in the statistically complete sample of flat-spectrum JVAS/CLASS sources of 11 670 sources. A simple Press–Schechter analysis is performed. For singular isothermal sphere lenses the lack of multiple image systems is inconsistent with the currently favoured cosmologies with     at the 4.2 σ level. Cored isothermal lenses reduce the expected number of lens systems and we suggest that the most probable interpretation of our results is that the surface mass density of groups and clusters of galaxies is not high enough to cause multiple imaging and the presence of the mass concentrations associated with individual galaxies is required to produce image separations such as those in B0957+561.