白银厂黄铁矿型铜、多金属矿床综合勘查模型   总被引：1，自引：0，他引：1  

李百祥 《甘肃地质》1994,3(1):90-95

在综合以往大量资料的基础上，补做钻孔原生晕、物性和物化探综合剖面工作，经理论模型正演，归纳概括出白银厂黄铁矿型铜、多金属矿床、矿田地质—地球物理—地球化学综合勘查模型，并对矿床、矿田按剥蚀程度不同分别提出预测标志。  相似文献   

从第55届EAEG年会看勘探地球物理发展方向     

李金铭 《地球物理学进展》1994,9(3):45-50

本文根据笔者在第５５届ＥＡＥＧ会议期间了解到的情况，对勘探地球物理在石油能源、固体矿产、水文地质、工程地质和环境地质等领域的进展作了综述，指出了今后的重点研究课题和发展方向。  相似文献   

大地测量与地球动力学─兼述它与地球物理学的联系     

张赤军 《地球物理学进展》1995,(4)

随着近代观测和实验技术的发展，人们越来越重视对地球运动及其机理的认识，并注意到大地测量学与地球物理学和地球动力学的联系与渗透。本文将对以上三者的联系以及大地测量学在监测地球运动和研究地球动力事件中的作用作一综述，并对近年国内外这方面的研究进展作一介绍。  相似文献   

Identification of buried sinkholes using refraction tomography at Ft. Campbell Army Airfield,Kentucky     

I. Camilo Higuera-Díaz  Philip J. Carpenter  Michael D. Thompson 《Environmental Geology》2007,53(4):805-812

Karst aquifers are highly susceptible to contamination, with numerous points of entry for contaminants through recharge features such as sinkholes, swallow holes and solutionally enlarged fractures. These recharge features may be filled or obscured at the surface, requiring the use of geophysical or remote sensing techniques for their identification. This study uses seismic refraction data collected at the Ft. Campbell Army Airfield (CAAF), Kentucky, USA, to test the hypothesis that refraction tomography is a useful tool for imaging bedrock depressions beneath thick overburden (greater than 20 m of unconsolidated sediment). Southeast of the main taxiway of CAAF seismic velocity tomograms imaged a bedrock low, possibly a closed depression, at a depth of 25 m that had been earlier identified through delay-time analysis of the same refraction data. Tomography suggests the bedrock low is about 250-m wide by 10-m deep at its widest point. High rates of contaminant vapor extraction over the western extension of this feature suggest a high concentration of contaminants above, and within, this filled bedrock low, the base of which may contain solutionally enlarged fractures (i.e. karst conduits) that could funnel these contaminants to the upper or lower bedrock aquifers. This study thus demonstrates the viability of seismic refraction tomography as a tool for identification of filled sinkholes and bedrock depressions in karst areas.  相似文献   

云南麻栗坡新寨锡矿物化探异常特征   总被引：3，自引：0，他引：3  

李文尧 《云南地质》2002,21(1):72-82

新寨锡矿是物化探扫面发现的大型锡石硫化物矽卡岩型矿床，高磁，高激电率，低电阻率异常，原生晕Sn,W,Cu,Zn,As,B,Ag,Cd,Be,Bi,In,F(Mo,Ge,Co)等元素异常，次生晕Sn,Cu,Zn,As,B等异常，总结地球物理化学特征，对滇东南寻找同类矿床具有重要指导意义。  相似文献   

用于地球物理反演的均匀设计优化算法   总被引：12，自引：4，他引：12       下载免费PDF全文

纪晨  姚振兴 《地球物理学报》1996,(2)

将均匀设计、模拟退火和单纯形方法相结合，提出一种全局优化迭代算法．数值模拟表明，它具有搜索速度快、搜索能力强和不需要求导数的特点，可用于地球物理反演研究．  相似文献   

An automatic radon probe for earth science studies     

M. Monnin  J. L. Seidel 《Journal of Applied Geophysics》1998,39(4):209-220

A field instrument designed for continuous radon measurement is described. It is based on a solid state electronic sensor that is housed in a rugged casing that also contains its associated electronics. This lightweight device is designed for selective counting of α-decays with recorded count values over specified intervals being stored within the device. Real time data processing to reject spurious values is automatically performed by the instrument. Data are downloaded by means of a handheld or a laptop computer. The energy provided by alkaline batteries ensures 2 months of continuous recording in the field. Example of radon anomalies are exhibited.  相似文献   

The main structure and tectonic features of the Chernorud-Mukhor site on the western shore of Lake Baikal from TEM and SP measurements     

Nikolai Kozhevnikov  Bülent Tezkan   《Journal of Applied Geophysics》1998,39(4):237-250

Transient electromagnetic (TEM), self-potential (SP) and geoelectrical mapping measurements were carried out at the Chernorud-Mukhor site in the Priolkhonje area on the western shore of the Lake Baikal. All measurements were made along several profiles across the main strike of the regional Primorsky fault. TEM measurements were carried out in a time range from a few tens of microseconds to several tens of milliseconds. The most important result of the 1D modelling of TEM soundings is the discovery of nearly horizontal boundaries that divide high resistive overlying and well conducting underlying rocks. The resistivity of the former is in the range from 100 Ωm to 1000 Ωm, while the resistivity of the latter varies from less than 1 Ωm to several tens of Ωm. This good conductive zone could also be verified by geoelectrical mapping using Schlumberger array (AB/2=100 m). Due to high conductivity of the underlying rocks only the upper boundary of the conductive layer could be determined by TEM soundings. A regional SP anomaly with amplitude of about −450 mV has also been observed above the low resistivity zone indicating the electron nature of its conductance. Geologically, the conductive zone is represented by a graphite-bearing layer within the region of archean rocks. Since that layer extends over a large area, it may be used as a key in studying structures and tectonics of the Priolkhonje area. A 1D TEM geoelectric section shows a wide, gently sloping syncline as a probable base structure of the Chernorud-Mukhor site. Neotectonic faults divide the syncline into vertically displaced blocks that form a wide complicated graben with a total amplitude of about 250 m.  相似文献   

An Approach to a Visual Language for Convective Fluid Flows: Visualization of Geophysical Simulations     

R. Zia  D. A. Yuen  T. A. Cortese  A. P. Vincent  S. Balachandar 《Visual Geosciences》1998,3(1):1-19

It was known that deep within numbers and binary data from simulations of geophysical convective flows resided various patterns. Two models of convective fluid flows were being considered. One was a model of two-dimensional (768 × 256) air convection with finite Prandtl number of one and Rayleigh number of 10⁸−10¹⁰, and another was a model of three-dimensional (up to 120 × 120 × 90) mantle convection with infinite Prandtl number and Rayleigh number of 10⁶−10⁸. Clearly, phenomena existed which superceded each individual dimensionless computer model to provide a piece of information regarding actual fluid flows. The problem was how to find, prove, and communicate these patterns and phenomena for convection simulations with gigabytes of data. In a search for such an analytical and communicative tool, the alternative of visualization was considered. The need for visualization was recognized and discussed. Then, utilizing both two- and three-dimensional models of high Rayleigh number convection, basic techniques of style and content were developed. Applications of the visualization techniques were designed utilizing IBM’s Data Explorer in order to create communicative images and movies, and after the applications, the problems of data storage and transfer became apparent. Throughout the process though, it became clear how important the language of vision actually could be in the geophysics community. In a field in which words such as plumes and internal waves have in ways replaced mathematics as the basic language for science, there is a need for another resource, another language-the visualization of convective fluid flows.  相似文献   

Hydrocarbon lakes on Titan     

Giuseppe Mitri  Adam P. Showman  Ralph D. Lorenz 《Icarus》2007,186(2):385-394

The Huygens Probe detected dendritic drainage-like features, methane clouds and a high surface relative humidity (∼50%) on Titan in the vicinity of its landing site [Tomasko, M.G., and 39 colleagues, 2005. Nature 438, 765-778; Niemann, H.B., and 17 colleagues, 2005. Nature 438, 779-784], suggesting sources of methane that replenish this gas against photo- and charged-particle chemical loss on short (10-100) million year timescales [Atreya, S.K., Adams, E.Y., Niemann, H.B., Demick-Montelara, J.E., Owen, T.C., Fulchignoni, M., Ferri, F., Wilson, E.H., 2006. Planet. Space Sci. In press]. On the other hand, Cassini Orbiter remote sensing shows dry and even desert-like landscapes with dunes [Lorenz, R.D., and 39 colleagues, 2006a. Science 312, 724-727], some areas worked by fluvial erosion, but no large-scale bodies of liquid [Elachi, C., and 34 colleagues, 2005. Science 308, 970-974]. Either the atmospheric methane relative humidity is declining in a steady fashion over time, or the sources that maintain the relative humidity are geographically restricted, small, or hidden within the crust itself. In this paper we explore the hypothesis that the present-day methane relative humidity is maintained entirely by lakes that cover a small part of the surface area of Titan. We calculate the required minimum surface area coverage of such lakes, assess the stabilizing influence of ethane, and the implications for moist convection in the atmosphere. We show that, under Titan's surface conditions, methane evaporates rapidly enough that shorelines of any existing lakes could potentially migrate by several hundred m to tens of km per year, rates that could be detected by the Cassini orbiter. We furthermore show that the high relative humidity of methane in Titan's lower atmosphere could be maintained by evaporation from lakes covering only 0.002-0.02 of the whole surface.  相似文献