放射性测量技术在油气勘查中的应用

本文介绍的油气勘查中的放射性测量，是一种油气普查新方法。它是利用油田上出现的负异常（或叫偏低场），反映了油气田的大体轮廓的基本原理进行的。前人及作者都取得了一定的工作成果。虽然取得了初步效果，但对机理等问题仍需进一步研究和完善。     

璜山金矿找矿模式及应用

诸暨璜山金矿是除治岭头以外浙江省第二金矿,它的找矿模式为"三高两低一复合"的找矿模式,即高金晕、高极化率、高磁场跳跃、低电阻率、低电位和北东断裂与北东东断裂复合处是成矿最有利部位.在其附近仍有类似成矿部位,有望扩大远景.     

1：2．5万沟系次生晕地球化学找矿方法探讨

从系统论的观点出发，将1：2．5万沟系次生晕地球化学找矿方法的室内布样，野外采样，室内异常圈定与评价和室外异常查证4个阶段看作一个有机的整体，在工作中，从布样阶段开始直至异常评价结束的每一个阶段都考虑后续的各个阶段可能会出现的问题，并采取相应应对措施，从布样到野外异常查证都注意地质信息和化探信息的相结合，从而总结出一套简便快捷，行之有效的野外工作方法，经过多年的实践和完善，该方法已在野外工作中发挥很好的效益。     

层间氧化带砂岩型铀矿矿物晕的非常规探测方法

本文以层间氧化带砂岩型铀矿矿物晕的一般特征为依托，介绍几种层间氧化带砂岩型铀矿矿物晕的非常规探测方法。     

弥散度及其在地下水污染模型中的作用

弥散理论是污染质在含水层中运移模型的基本理论.但在实际应用中存在着不少问题和争议.本文对污染质在含水层中运移的弥散作用进行了分析探讨.并应用MOC水质模型对弥散参数的作用进行了分析,证明了在一般情况下,污染质在含水层中的运移主要受对流作用控制,弥散参数的变化对水质模型结果的影响相对较小.在特定的水文地质条件下,弥散作用对污染质的运移是重要的.     

Dark haloes of spiral galaxies: ISO photometry

We exclude hydrogen-burning stars, of any mass above the hydrogen-burning limit and any metallicity, as significant contributors to the massive haloes deduced from rotation curves to dominate the outer parts of spiral galaxies. We present and analyse images of four nearly edge-on bulgeless spiral galaxies (UGC 711, NGC 2915, UGC 12426, UGC 1459) obtained with ISOCAM (The CAMera instrument on board the Infrared Space Observatory ) at 14.5 and 6.75 μm. Our sensitivity limit for detection of any diffuse infrared emission associated with the dark haloes in these galaxies is a few tens of μJy per 6 × 6 arcsec² pixel, with this limit currently set by remaining difficulties in modelling the non-linear behaviour of the detectors. All four galaxies show zero detected signal from extended non-disc emission, consistent with zero halo-like luminosity density distribution. The 95 per cent upper limit on any emission, for NGC 2915 in particular, allows us to exclude very low mass main-sequence stars ( M  > 0.08 M⊙) and young brown dwarfs (≲1 Gyr) as significant contributors to dark matter in galactic haloes. Combining our results with those of the Galactic microlensing surveys, which exclude objects with M  < 0.01 M⊙, excludes almost the entire possible mass range of compact baryonic objects from contributing to Galactic dark matter.     

The globular cluster system of the Sagittarius dwarf spheroidal galaxy: the age of Terzan 8

We present deep V - and I -band CCD photometry of the globular cluster Terzan 8, recently found to be a member of the globular cluster system of the Sagittarius dwarf spheroidal galaxy. We accurately estimate the metallicity of Terzan 8, and provide the first direct determination of the colour excess toward this cluster. Our robust age estimate confirms that this cluster is indeed coeval with typical Galactic globulars of comparable metal content, and thus it is probably significantly older than at least two other Sagittarius clusters, Terzan 7 and Arp 2. The implications of this result on the star formation history of the Sagittarius galaxy are briefly discussed.     

Numerical studies on the structure of the cosmic ray electron halo in starburst galaxies

The structure of the cosmic ray electron halo of a starburst galaxy depends strongly on the nature of galactic wind and the configuration of the magnetic field. We have investigated these dependencies by solving numerically the propagation of electrons originating in starburst galaxies, most likely in supernova remnants. The calculations are made for several models for the galactic winds and for the configuration of the magnetic fields for comparison with observations. Our simulation of a quasi-radio halo reproduces both the extended structure of ∼9 kpc and the subtle hollow structure near the polar region of the radio halo that are observed in the starburst galaxy NGC 253. These findings suggest the existence of strong galactic wind in NGC 253.      

山东金青顶金矿床控矿构造特征及深部预测

金青顶金矿床位于山东牟平-乳山金矿带将军石-曲河庄断裂的南端,矿床围岩为昆嵛山花岗岩,属含金石英脉型金矿。本文通过矿床地质特征、围岩蚀变以及控矿构造特征等方面的研究,认为与成矿有关的构造活动至少划分为4期,基本控制着矿体的定位与分布。深部地球化学原生晕研究表明,矿体在垂向上具有明显的地球化学分带性,且在已知矿体下方出现近矿晕、前缘晕及尾晕特征指示元素构造叠加晕强度升高趋势。结合矿体在断裂中分布的规律以及原生晕特点,对金青顶矿床深部第二富集段进行了预测,推断在-1100m下有第二金富集段存在,且具有很大的经济价值。     

新疆东天山红石金矿床原生晕特征与矿体叠加模型

红石金矿床是新疆东天山康古尔塔格金矿带中的代表性矿床之一。通过对其地表、已开采中段及部分钻孔的岩石系统采样分析和计算统计,研究了各指示元素在不同位置的组合特征。结果表明:指示元素中Au、Ag密切相关,其他元素组合复杂多变,反映了成矿成晕的多期性、多阶段特点。结合实际勘查资料,采用多种计算方法,建立了矿床原生晕轴向分带模式,即矿床轴向分带(自上而下)为Bi-Mo-Hg-Zn-Pb-Ag-As-Cu-Sb-Au。利用不同中段的7个分带评价值指标确定了矿体的叠加模型。