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1.
地球物理勘探在地学研究中起到十分重要的作用,其方法种类较多,在各类物探方法的具体工作中,了解相应方法所能探测到异常体的深度范围,对物探工作的开展十分重要.本文通过对当前地面重力与磁法、常用的电法、放射性方法以及常用的各类航空物探方法在找矿等方面的众多实例勘探深度的研究,总结归纳了现阶段各种常用地球物理方法的勘探深度.总结发现目前重力勘探的找矿深度一般在400 m左右,最大可达到897 m;在地质构造研究方面勘探深度在10~20 km之间,结合其他物探方法最深可达到150 km.目前磁法勘探找矿深度一般在400~500 m,最大深度可达到989 m.电法勘探分支方法较多,多数电法的勘探深度在200~300 m;瞬变电磁法的勘探深度集中在300~400 m,最大可以达到1500 m;大地电磁法的勘探深度集中在700~800 m,最大可达到1800 m以上.放射性勘探主要集中于地表至200 m以浅的放射性矿产勘探.并以典型实例说明各种物探方法可达到的最大深度,研究了影响各种地球物理方法勘探深度的因素,根据总结得到的各类地球物理方法勘探深度,对不同物探方法所适用的地质研究领域与深部找矿方向进行了展望,为实际工作的设计提供参考.  相似文献   

2.
对不同埋深花岗岩采用重力法、电法和电磁法、地震法等地球物理勘探方法的结果差异性如何?本文以广东大亚湾花岗岩为例,先后开展了重力法、高密度电法、地震折射法、可控源音频大地电磁法(CSAMT)等4种不同方法,探测中微子场地断层破碎带、花岗岩与沉积岩接触带、风化壳厚度、地下水埋深等与隧道工程设计方案和围岩稳定性密切相关的地质条件.地球物理勘探以岩层物性(电阻率、波速和密度等)为基础,这些特征与岩性及地下水状态相关.同时相同物性特征对应不同岩层和含水状态,因而物探结果具有多解性.在工作中采用多种物探方法进行了相互补充验证.勘探结果比较后发现,对浅表50 m以内风化壳厚度,以人工重锤为激发震源的地震折射法效果较好,对风化壳分带和厚度达100多米的风化囊,高密度电法探测效果较好,而对于深大断裂或密闭断裂,重力法和电磁法效果较好.这四种不同物探方法结果的综合分析,对全面深入认识花岗岩地质条件提供了依据,其结果得到了钻探和隧道工程施工开挖揭露的验证.  相似文献   

3.
综合物探方法在滇池补水工程中的应用   总被引:1,自引:1,他引:0  
本文介绍了包括地震、瞬变电磁法、高密度电法、高频大地电磁法等在内的多种物探方法在滇池补水工程岩土工程勘察中的应用情况.通过选择其中一种或几种物探方法分别应用在河床冲积层、断层带和岩溶探测上,使得物探方法在对物探异常的分辨上能够相互印证,提高了解释成果的可靠性,在探测深度上采用适合浅部勘探的物探方法和适合深部勘探的物探方...  相似文献   

4.
应用高密度电法、地质雷达及面波测试等综合地球物理方法,解决广西兴安灵渠渗水治理工程中地质调查的实际问题.采用高密度电法探测场区地层情况及秦堤渗水病害情况;地质雷达方法探测探明了场区表层土体密实度及空洞情况;面波测试进行了场区覆盖层速度分层及不良地质现象判定.最后,综合分析三种物探方法的探测结果并将其与后期钻探成果进行了对比验证.结果表明:综合物探探测成果与后期钻探验证结果一致.工程实践表明,采用多种物探方法相互印证,对比解译分析在工程地质调查中是必要的也是十分有意义的.  相似文献   

5.
超高密度电阻率法是Australia ZZ Resistivity Imaging研发中心积近十年的研究成果提出的全新的电阻率法勘探理念,是电法勘探从手工时代向计算机时代的一次跨越式发展,采用一次布极,采集所有可能组合电极间的电位信息,信息量较常规电法在信息量上翻了40倍以上,并且避开视电阻率概念,利用处理软件直接反演获取断面真电阻率值,针对目前还没有行之有效的地面物探方法可以勘探清楚的土洞、煤窑采空区和岩溶等复杂地质问题,我们采用该方法分别对机场岩溶和土洞、煤矿运煤巷道、隐伏小煤矿采空区和复杂地质病害隧道进行了试验勘探,经钻探验证,准确率在60%以上,达到国内领先水平,取得了较好效果,对复杂地质的工程勘探具有一定参考价值.  相似文献   

6.
针对山区长埋深隧洞勘测技术的研究,是近年来我国隧洞地质勘查中的研究热点,然而传统的钻探等手段在多山区域有很大的局限性,因此,近些年来地球物理勘探方法逐渐面向工程勘探,而单一的物探方法往往在异常判断方面存在局限性,鉴于此在工程勘探中往往运用多种地球物探方法相结合,可以在一定程度上减小了单一物探方法的多解性,提高物探解释的质量以及精度.本文以南水北调某工程为例,在某受水段分别布置了大地电磁法、地震浅层反射物探方法,其中大地电磁法主要用于辅助查明隧洞覆盖层厚度、地层岩性、隐伏构造、地下水位等工程地质条件,地震浅层反射用于查明小规模的地质构造(小断层、溶洞等)的勘查,经过这两种方法的结合,有效的查明了工程受水区的基本地质情况.  相似文献   

7.
综合物探方法在滑坡等地质灾害的勘探中发挥着重要的技术作用。这里以河南省某地滑坡勘探为例,利用高密度电阻率法和地质雷达法等综合物探方法,分析两种物探方法的技术原理、联合解释,并结合地质钻探、地质调查等资料,查明该场地滑坡体的分布情况。结果表明,综合物探方法能有效地减少物探的多解性,提高成果解释精度,其综合物探解释成果与地质情况较为吻合,显示出综合物探方法在滑坡等地质灾害勘探中的重要作用。最后,对综合物探方法及综合解释进行了简要的总结和展望。   相似文献   

8.
独山半坡锑矿石与围岩物性差异并不特别显著、矿体埋深较深,常规的物探方法无法满足目前的勘探要求.可控源音频大地电磁法(CSAMT)具有勘探深度范围大、分辨率高、地形影响和高阻层的屏蔽作用小,立体观测等特征,在深部找矿中发挥着重大的作用.本文首先概述了CSAMT基本原理和工作方法,在全面掌握了地质资料、物性参数的基础上,对独山半坡锑矿外围开展了CSAMT法勘探,通过应用Occam算法对CSAMT实测数据进行反演,成功地圈定了电阻率异常区域,有效地指导钻孔设计.物探异常钻探见矿,验证了CSAMT方法在深部找矿工作中的有效性,可为寻找同类深部锑矿提供指导和借鉴意义.  相似文献   

9.
地球物理方法在金属矿深部找矿中的应用及展望   总被引:4,自引:3,他引:1  
地球物理勘探方法对深部隐伏矿床找寻及预测具有很强的指导性,在近年来国内外找矿工作中(特别是隐伏矿的预测)取得了很好成效.本文着重论述了重、磁、电、震、测井等地球物理方法在金属矿深部找矿中的应用特点和成果.事实表明,不同物探方法在找矿过程中有不同的特点和适用条件,要根据具体找矿对象特征,综合运用这些方法,并结合地质与地球...  相似文献   

10.
综合物探方法在人工洞室探测中的应用效果分析   总被引:1,自引:0,他引:1  
随着人们对地下溶洞和人工洞室的探测精度的要求越来越高,单一的物探方法并不能满足高精度勘探的要求.本文以对某地一人工洞室投入磁法、电法、地震波法的探测结果为例,通过对探测结果的对比分析,说明在探测此类问题中如何合理地选择物探方法,对后期的工程建设有一定的指导作用.  相似文献   

11.
The data on geomagnetic reversals are compared with the changes in the organic world and with the lower-mantle plumes. The times of the formation of plumes and the times of their appearance on the Earth’s surface relate to the intervals characterized by the different frequencies of geomagnetic reversals, i.e., there is no interrelation between the formation of plumes and the frequency of the changes in the geomagnetic field polarity. At the same time, a certain synchronism is observed between the frequency of the geomagnetic reversals and the boundaries of the biostratigraphic ages, i.e., the changes in the organic world in the long-period range. A hypothesis is proposed, which explains the change in the sign of the geomagnetic field by the combined effect of the irregular rotation of the internal core relative to the mantle and the changes in the slope angle of the axis of the Earth’s rotation, which, in turn, results in synchronous events on the Earth’s surface: the rates of changes in the organic world.  相似文献   

12.
Summary The maintenance of the axisymmetric component of the flow in the atmosphere is investigated by means of a steady-state, quasi-geostrophic formulation of the meteorological equations. It is shown that the meridional variations in the time-averaged axisymmetric variables can be expressed as the sum of three contributions, one being due to the eddy heat transport, another to the eddy momentum transport, and a third to the convective-radiative equilibrium temperature which enters the problem through the specification of a Newtonian form of diabatic heating. The contributions by the large scale eddies are evaluated through the use of observed values for the eddy heat and momentum transports.The contributions from each of the three forcing mechanisms to the temperature and zonal wind fields are invstigated individually and found to be of about equal importance. The sum of the three contributions are also presented for the temperature, the zonal wind, the stream function associated with the mean meridional circulation and the corresponding vertical motion. Although the results fail to reproduce the main observed features of the lower stratosphere, they are found to be in good agreement with observations in the middle latitude troposphere. At any pressure level, for example, the computed mean zonal wind has a jet-like profile and the axis of the jet is found to slope to the south with height, as observed in the atmosphere.Based in part on a thesis submitted by the first author as partial fulfillment of the requirements for the Ph.D. degree at the University of Michigan. — Publication No. 194 from the Department of Meteorology and Oceanography, The University of Michigan.  相似文献   

13.
Summary The author mentions the aims of the World-wide gravity project he established in the Ohio State University in Columbus, in 1950. He outlines the practical procedure of the gravimetric computations of the undulationsN and the vertical deflection components and and emphasizes that only by the global international cooperation and additional gravity observations at sea carried out during the last decade it has been possible to gather to Columbus the needed gravity material. Since there exist still large gravimetrically unsurveyed areas it is of vital significance to study what gravity anomalies are best to be used for these regions. The given figures concerning the accuracy of theN, and , estimated theoretically and obtained in practice, indicate that in the gravimetrically well surveyed parts of the world like in Europe and the United States we can get gravimetrically on basis of existing gravity material theN-values with accuracy of about 5–10 meters, and and with the accuracy of about 1. The geoid undulationsN are already computed in Columbus for more than 6000 points of the northern hemisphere. The sample maps show the interesting geoid of Europe and vicinity between the latitudes 60° and 30° and longitude 5° W and 30° E, drafted on basis of more than 1000N-values computed at the corners of 1°×1° squares. It is interesting to realize that the geoid undulations in all this area are positive, the extreme values being between 40 and 50 meters. The geophysical significance of the geoid maps of this kind is pointed out.  相似文献   

14.
15.
陈伯舫 《华南地震》2004,24(4):8-10
综合APIA、HONOLULU、PAMATAI 3个地磁台三分量的11年周期变化的形态后,可定性地提出该变化源于内场。如内源为核幔边界的电涡流,则其中心点应位于3台之间。  相似文献   

16.
The global database on the paleointensity, containing determinations of the virtual dipole moment (VDM) for a stable (normal) regime of the geomagnetic field in a time interval of up to 3.5 Ga, is supplemented by new VDM determinations and analyzed. The field generation process started no later than 3–3.5 Ga (earlier data are absent) at the stage of the Earth’s core formation. Since that time, the dipole value has differed from its present value by no more than an order of magnitude, and the deviations that have already been detected tend toward smaller values. The distribution of VDM values in the time interval 0–400 Ma is bimodal, which apparently reflects the presence of two different generation levels of the geomagnetic field distinguished by a relatively large value (close to the present field value) and a relatively small value (approximately half as large as the present value). The total duration of decreased VDM values appreciably exceeds that of increased VDM values (179.1 and 28.6 Myr, respectively). On the whole, data on the paleointensity do not contradict the hypothesis about the dipole nature of the field over the last 400 Myr; however, the number of determinations at high paleolatitudes is too small to draw decisive conclusions on the validity (or invalidity) of the dipole field approximation based solely on paleointensity data.  相似文献   

17.
Until recently, the existing data prevented the geophysicists from accurately dating the Bysy-Yuryakh stratum, which outcrops in the middle reach of the Kotuy River, constraining the time of its formation to a wide interval from the end of the Late Cambrian to the beginning of the Silurian. The obtained paleomagnetic data unambiguously correlate the Bysy-Yuryakh stratum to the Nyaian regional stage and constrain its formation, at least a considerable part of it, by the Tremadocian. This result perfectly agrees with the data on the Bysy-Yuryakh conodonts studied in this work and yields a spectacular example of the successful application of paleomagnetic studies in solving important tasks of stratigraphy and, correspondingly, petroleum geology. Within the Bysy-Yuryakh stratum, we revealed a large normal-polarity interval corresponding to the long (>1 Ma) period when the geomagnetic reversals were absent. This result, in combination with the data for the Tremadocian and Middle–Upper Cambrian sequences of the other regions, indicates that (1) the rate of occurrence of the geomagnetic reversals on the eve of the Ordovician Moyero superchron of reversed polarity was at most one reversal per Ma; (2) the superchron does not switch on instantaneously but is preceded by a certain gradual change in the operation conditions of the dynamo mechanism which, inter alia, manifests itself by the reduction of the frequency of geomagnetic reversals with the approach of the superchron. This finding supports the views according to which a process preparing the establishment of the superchrons takes place at the core–mantle boundary.  相似文献   

18.
The nutations of the planets Mars andEarth are investigated and compared. Alarge number of interior structureparameters are involved in the nutationcomputations. The comparison between the observations and the computationsprovides several constraints on these parmeters andtherefore allows a better understanding of the physics of the interior of theplanet. For the Earth, the high precision of the observations of the nutationshas led to a very good determination of interior properties of the planet. ForMars, observations of nutations are not yet available, and we review how theamplitude of the Martian nutations depends on the hypotheses consideredfor its interior. Although Mars is very similar to the Earth, its interior is not well known;for example, we don't knowif its core is liquid or solid. Only if the core is liquid,the Free Core Nutation (FCN) normal mode exists and can alter the nutationswhich are close to the resonance. From the observed geoids, it is known thatboth planets are not in hydrostatic equilibrium. The departure is larger forMars than for the Earth, and consequently, the implication of considering a convective mantle instead of a mantle in hydrostatic equilibrium described byClairaut's equation for the initial equilibrium state of the planet is largeron the Martian nutations than on the Earth nutations. The consequences of theuncertainty in the core dimensions are also examined and shown to be of a veryhigh influence for Mars if the core is liquid, due to the potential changes inthe FCN resonance. The influence of the presence of an inner core, which isknown to exist for the Earth, could be more important for Mars than for theEarth if the inner core is large. Due to the presence of Tharsis on Mars, thetriaxiality of this planet has, additionally, larger effects than on Earth.  相似文献   

19.
20.
Geomagnetism and Aeronomy - The evolution of the magnetic configuration in the solar corona is studied. The curvature of the K-corona helmets obtained from an analytical approximation of the...  相似文献   

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