云南巍山—永平矿集区流体地质填图的理论与实践

流体地质填图是一种全新的地质调查及找矿方法。本次研究选择云南巍山－永平矿集区进行流体地质填图试验，研究了矿集区的控矿地质要素、各种主要的矿床（点）特征、成矿流体子系统及流域、流体的盐度与均一温度、流体的气液相成分、微量元素含量、稳定同位素特征及成矿流体的浓集中心。得到的流体地质图基本反映了本区成矿流体的性质与状态，反映了两个成矿流体子系统的基本特征，圈字了2个成矿流体子系统的流域范围及7个成矿流体浓集中心。这些浓集中心与已知矿化点分布、化探异常及有利的地质条件基本吻合，成为该区进一步找矿预测的重要依据之一。本项目的实践表明，流体地质填图不失为一种有效的找矿手段。     

当代世界地质调查工作发展趋势

20世纪80年代以来，经济全球化的发展、高新技术的广泛应用、世界人口的迅速增长和环境问题的日益严峻，对地质调查工作产生了巨大的冲击，地质调查的驱动机制、主要任务和工作内容、技术手段、服务意识等都发生了很大的变化。总体趋势为：需求驱动——地质调查工作的驱动机制由传统的供给驱动型向需求驱动型转变；领域拓宽——地质调查的研究领域不断拓展，从以寻找、发现矿产资源为主的矿产资源型转变为兼顾资源与环境保护、灾害减轻的资源与环境并重的社会型；技术先导——地质调查的技术手段发生了根本性变化，地质调查传统的“老三件”正逐渐被“新三件”所替代；服务优先——地质调查的服务意识不断增强。     

多目标地球化学调查在成都平原的实践

通过在中国西部地区成都平原首次开展的多目标地球化学调查，研究了深层样元素的基准值及浅层样元素的分布特征，并利用元素的分布特征判断隐伏构造和隐伏岩体；探讨了在农业地质、环境污染、人体健康、天然气预测、pH值计算等多目标的地球化学研究。     

北山戈壁荒漠地区1：5万植物地球化学测量效果

北山戈壁荒漠景观区土壤垂直剖面不存在通常的A、B、C分层结构，且掺杂有大量风成沙。在公婆泉地区开展1：5万常规地球化学测量方法研究的同时，进行了植物地球化学测量试验研究。研究表明，两种方法的主要指示元素异常有很好对应性，红沙是我国西部干旱荒漠广大地区开展植物地球化学测量的一种良好采样对象。     

遥感技术在高寒山区1:25万区域地质调查中的应用研究

针对高寒山区1：25万区调野外工作条件差、时间短，植被覆盖度低、遥感影像质量好的特点，提出了遥感影像解释、遥感标志剖面解译新概念，以及不同工作区用不同大法的新思路。研究、实践认为，利用遥感技术开展高寒山区区域地质调查能减少野外工作量，缩短周期，节约经费，提高调查质量和精度。     

义敦成矿带铜银铅锌锡矿产资源调查评价进展与潜力

义敦成矿带地处独特的大地构造部位，经历了复杂的地质构造演化和强烈的岩浆活动，成矿条件优越，矿产资源丰富。1999年实施国土资源地质大调查以来，相继发现了普朗、松诺、卓玛斑岩铜矿；砂西、热朗泽、夏隆等银铅锌矿；热隆、脚根玛锡矿；打马池觉铜金矿等一批具有重要找矿前景的矿床(点)。该地区矿产资源勘查工作程度低，蕴藏着较大的找矿潜力，有望成为国家级重要的有色及贵金属矿产勘查和开发基地。     

高密度电法勘探在岩溶查找中的应用

介绍了武汉市汤逊湖污水处理厂厂址的地质概况和地球物理特征，以及高密度电法勘探的施工方案，分析了视电阻率异常特征，并说明了其异常验证情况。高密度电法勘探结果表明该区存在溶洞，为施工提供了决策依据，建议在有溶洞的地段采取相应措施，以防止工程建设后发生地质灾害。     

陕西省地下水水质监测发展探析

本文针对陕西省地下水水质监测控制范围局限于农灌区，监测项目单一的现状，通过分析研究，提出水质监测的发展思路，剖析实现新思路的相关条件。     

全站仪机载导线测量程序开发研究

介绍了全站仪机载程序开发的重要性和必要性，基于Leica公司TPS1000／1100系列全站仪机载程序开发工具——GeoBASIC，阐述了机载导线测量程序开发的技术关键，所开发的程序达到了预期的效果，满足了用户的需求。     

The electrical structure of the Slave craton

The Slave craton in northwestern Canada, a relatively small Archean craton (600×400 km), is ideal as a natural laboratory for investigating the formation and evolution of Mesoarchean and Neoarchean sub-continental lithospheric mantle (SCLM). Excellent outcrop and the discovery of economic diamondiferous kimberlite pipes in the centre of the craton during the early 1990s have led to an unparalleled amount of geoscientific information becoming available.

Over the last 5 years deep-probing electromagnetic surveys were conducted on the Slave, using the natural-source magnetotelluric (MT) technique, as part of a variety of programs to study the craton and determine its regional-scale electrical structure. Two of the four types of surveys involved novel MT data acquisition; one through frozen lakes along ice roads during winter, and the second using ocean-bottom MT instrumentation deployed from float planes.

The primary initial objective of the MT surveys was to determine the geometry of the topography of the lithosphere–asthenosphere boundary (LAB) across the Slave craton. However, the MT responses revealed, completely serendipitously, a remarkable anomaly in electrical conductivity in the SCLM of the central Slave craton. This Central Slave Mantle Conductor (CSMC) anomaly is modelled as a localized region of low resistivity (10–15 Ω m) beginning at depths of 80–120 km and striking NE–SW. Where precisely located, it is spatially coincident with the Eocene-aged kimberlite field in the central part of the craton (the so-called “Corridor of Hope”), and also with a geochemically defined ultra-depleted harzburgitic layer interpreted as oceanic or arc-related lithosphere emplaced during early tectonism. The CSMC lies wholly within the NE–SW striking central zone defined by Grütter et al. [Grütter, H.S., Apter, D.B., Kong, J., 1999. Crust–mantle coupling; evidence from mantle-derived xenocrystic garnets. Contributed paper at: The 7th International Kimberlite Conference Proceeding, J.B. Dawson Volume, 1, 307–313] on the basis of garnet geochemistry (G10 vs. G9) populations.

Deep-probing MT data from the lake bottom instruments infer that the conductor has a total depth-integrated conductivity (conductance) of the order of 2000 Siemens, which, given an internal resistivity of 10–15 Ω m, implies a thickness of 20–30 km. Below the CSMC the electrical resistivity of the lithosphere increases by a factor of 3–5 to values of around 50 Ω m. This change occurs at depths consistent with the graphite–diamond transition, which is taken as consistent with a carbon interpretation for the CSMC.

Preliminary three-dimensional MT modelling supports the NE–SW striking geometry for the conductor, and also suggests a NW dip. This geometry is taken as implying that the tectonic processes that emplaced this geophysical–geochemical body are likely related to the subduction of a craton of unknown provenance from the SE (present-day coordinates) during 2630–2620 Ma. It suggests that the lithospheric stacking model of Helmstaedt and Schulze [Helmstaedt, H.H., Schulze, D.J., 1989. Southern African kimberlites and their mantle sample: implications for Archean tectonics and lithosphere evolution. In Ross, J. (Ed.), Kimberlites and Related Rocks, Vol. 1: Their Composition, Occurrence, Origin, and Emplacement. Geological Society of Australia Special Publication, vol. 14, 358–368] is likely correct for the formation of the Slave's current SCLM.