云南勐兴铅锌矿矿体空间特征及预测前景     

赵长江  高建国  王开林  丁秀芳 《云南地质》2008,27(4):496-501

借助ArcGIS软件的空间统计分析功能,对矿体主要参数进行分析,获得矿体空间特征。认为铅和锌品位具有明显的正相关,品位与厚度也属正相关。在此基础上对矿区找矿远景区进行初步圈定,为探矿工程的布置提供依据。  相似文献   

富宁阳文冲-广南菜子垣热液淋滤卡林型金矿区     

王泽传  王维刚  吴赵全 《云南地质》2008,27(3):309-314

金矿区构造活动具有多期性：加里东期及海西期在矿区形成的薄弱角度不整合面、近南北向平行的滑脱断层,是含矿热液的运移、沉淀的通道和空间。金矿床应属地下热液淋滤卡林型金矿床。  相似文献   

云南永胜宝坪浅源热液改造型铜矿地质及成因     

谭玉荣  秦培林  王学武  高建国 《云南地质》2008,27(3):357-361

宝坪铜矿赋存于三叠系下统腊美组中。矿体呈似层状,少量脉状,严格受北北西-北西向构造控制。矿床成因类型属浅源热液改造型铜矿床。  相似文献   

GIS软件符号功能特点   总被引：1，自引：0，他引：1  

杜伟  潘峰  胥兵 《云南地质》2008,27(3):371-375

讨论当前国内外GIS软件的符号功能及花纹图案填充功能的特点,指出实际应用中不足,为现有软件平台进行符号设计、编辑以及制图等提供参考。  相似文献   

红层泥岩水岩作用特征研究   总被引：1，自引：0，他引：1  

张永安  李峰  陈军 《工程地质学报》2008,16(1):22-26

红层是红色陆相沉积为主的碎屑沉积岩层,岩性以砂岩、泥岩、粉砂岩和页岩为主。该类岩层多为软岩与硬岩相间,呈互层状产出,层间结合力弱。受区域构造影响,岩层扭曲褶皱强烈,多中高倾角,结构面发育,有泥化现象。红层中的泥岩具有透水性弱、亲水性强,遇水易软化、塑变,抗风化能力弱,易崩解等特性。特别是遇水后岩体及结构面抗剪强度大幅度降低,并且具有遇水膨胀、失水收缩的工程特性。水岩作用对边坡的影响主要有,结构面遇水泥化导致楔形体失稳,泥岩塑性变形引起边坡蠕变,同时红层还具有很强的崩解性,边坡开挖后发生崩解等现象。  相似文献   

云南省兰坪县凤岩山铅锌铜多金属矿地质特征及成因探讨     

武龙祥  刘江波  张准  杨吉忠 《华南地质与矿产》2008,(1):49-54

凤岩山铅锌铜多金属矿位于兰坪断陷盆地中部,是云南省乃至全国重要的铅锌成矿区之一,具有良好的成矿条件和找矿前景。本文通过对矿区地质背景条件、地质特征、地球化学异常特征、矿体特征、矿石特征的分析的研究,认为矿床成因应为后期热卤水为主改造叠加形成的,属沉积-改造层控型矿床。  相似文献   

山区公路工程建设对地下水渗流的影响   总被引：1，自引：0，他引：1  

张林洪  王甦达  唐正光  吴华金  段翔  彭绍勇 《地质灾害与环境保护》2008,19(4):81-86

分别就公路路堤、路堑、半挖半填等路基结构和隧道结构对周围岩土体的渗透性、渗流路径、地下水位等方面的影响进行了分析,以对公路工程建设对地下水环境的影响和与水文地质有关的灾害和损害的分析评价有所帮助。  相似文献   

昆明滇池周围磷矿资源现状及开发前景   总被引：2，自引：0，他引：2  

薛步高 《化工矿产地质》2008,30(3)

云南磷矿探明储量居全国首位,滇池周围保有储量占全省保有储量68.64%。磷化工与磷复肥基地和国内最大露采矿山,均在此区域内。"优矿低用"、矿山规模化小、国营矿山效益差,均是发展中要解决的问题。合理开采富矿、发展磷肥要"湿、热并举"、实施"矿电联营"、政府给予优惠政策,是云南磷矿业可持续发展的重要举措。  相似文献   

Multi-cloud model (MCM) method and its applications to the study on asymmetric spectral profiles   总被引：1，自引：0，他引：1  

Xiao-Ma Gu  Jun Lin  Ke-Jun Li  Jing-Ping Dun 《Astrophysics and Space Science》1996,240(2):263-271

A method of multi-cloud model (MCM) is proposed in this paper in order to research asymmetric profiles of spectral line formed by solar discrete active objects aligned along the line-of-sight difection. Based on the MCM method, under the conditions of certain assumptions and approximations, the line-of-sight velocityV and three other physical parameter approximation values, (i.e. Doppler width _D , source functionS and optical depth at line center ₀) within different clouds may be derived simultaneously by fitting both profiles theoretical and observational. An application example of the method withm=3 shows that MCM method is suitable to measure the velocity fields of multi-object at the same time from their non-Gaussian profiles of complex. TheV and _D derived from the method are reliable,S and ₀ are approximation. An influence of the variations of initial values in the parameter on the solution is given as well.  相似文献   

A quantitative model of coherent,stimulated emission in astrophysical jets     

J. C. Wang  G. Z. Xie  J. Lin 《Astrophysics and Space Science》1994,213(2):257-271

On the basis of issues raised by observations of BL Lac objects and the qualitative jet model proposed by Bakeret al. in 1988, we have been led to consider the quantitative role of coherent, stimulated emission in jets and construct a new jet model of blazars in which a relativistic electron beam with an axial symmetric, power-law distribution is injected from the central engine into the jet plasma. We study quantitatively the synchrotron emission of the relativistic electron beams. Using the weak turbulent theory of plasma, we discuss the interaction between relativistic electron beams and jet plasma, and the roles of stimulated emission. The main results are:

1. The synchrotron emission increases sensitively with the increase of the angle between the direction of the beam and the magnetic field. When the direction of the beam is vertical to the magnetic field, the synchrotron emission reaches its maximum, i.e. the emitted waves are beamed in the direction of the jet axis. We suggest that radio selected BL Lac objects belong to this extreme classification.
2. The synchrotron emission of the relativistic beam increases rapidly with the increase of the Lorentz factor of the relativistic electron,γ, whenγ ≤ 22.5, then decreases rapidly with increase ofγ.
3. The stimulated emission also increases with increasing Lorentz factorγ of the relativistic electrons whenγ ≤ 35 and then decreases with the increasingγ. The maximum stimulated emission and the maximum synchrotron emission occur at different frequencies. Stimulated emission is probably very important and reasonable flare mechanism in blazars.
4. The rapid polarization position angle (PA) swings may arise from the interaction between the relativistic electron beam and the turbulent plasma.

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