赣南隆坪萤石矿床成矿流体特征及成矿模式探讨     

杨世文  丰成友  楼法生  许德如 《地质学报》2022,96(11):3886-3900

赣南兴国县隆坪大型萤石矿床位于大余 南城深大断裂西侧兴国 宁都萤石成矿带内，呈板状、似层状、脉状产于永丰复式岩体外接触带北东向硅化破碎带中。本文划分了兴国县隆坪萤石矿床的成矿阶段，通过流体包裹体岩相学、显微测温、激光拉曼成分分析和H O同位素研究，讨论了该矿床成矿流体性质、来源、演化与成矿模式。根据矿物穿插关系和矿相学特征，将隆坪萤石矿床划分为3个成矿阶段，即成矿早阶段(萤石 石英阶段)、成矿主阶段(石英 萤石阶段)和成矿晚阶段(萤石 方解石阶段)。流体包裹体类型主要为富液相两相包裹体，均一温度变化范围在111~374℃之间，盐度变化于0. 53%~3. 55%NaCleq之间 ，密度变化于0. 58~1. 02 g/cm3之间。包裹体成分以H2O为主。总体而言，成矿流体属于中低温、中低盐度、中低密度的NaCl H2O体系，但成矿早阶段存在高温、相对高盐度的流体端元(温度大于300℃，盐度为2. 0%~2. 7%NaCleq)，推断永丰复式岩体晚阶段岩浆热液参与早阶段萤石成矿作用，提供F的来源和热源。隆坪萤石矿床流体包裹体中的δDV SMOW和δ18OV SMOW值均较低，分别为-66. 8‰~-53. 1‰(平均值为-59. 5‰)和-5. 9‰~-3. 3‰ (平均值为-4. 6‰)，成矿流体主要来源于大气降水和地热水。成矿早阶段萤石沉淀机制主要为岩浆热液和大气降水混合与水 岩反应，而流体冷却作用是成矿主阶段和晚阶段萤石沉淀的主要机制。隆坪萤石矿床属断裂控矿、中低温热液裂隙充填型萤石矿床。  相似文献   

江西省丹霞地貌特征及其控制因素探讨     

陈留勤  郭福生  邵崇建  楼法生  李斌  黎广荣  郄海满  吴知勇  姜勇彪  刘富军 《地质学报》2022,96(11):4023-4037

江西省的丹霞地貌主要分布在30余个白垩纪红层盆地中，总共有228处，数量位居全国之首，以鹰潭市龙虎山世界地质公园的丹霞地貌最为典型和知名。根据形态特征，将江西省的丹霞地貌划分为山峰、陡崖、崩积体、峡谷、洞穴及其他微地貌等六大类。燕山构造旋回晚期（主要是白垩纪），在地壳伸展拉张的构造背景下，江西省形成了一系列北东走向的陆相断陷盆地，从盆地边缘到中心依次沉积红色冲 洪积扇相砾岩、河湖相砂岩和泥岩，在信江盆地的中部还发育沙漠相风成砂岩。红层岩相是丹霞地貌演变的基本物质基础，对丹霞地貌的分布具有重要影响。在喜马拉雅构造旋回中，这些红层被构造抬升、切割，随后在风化、流水侵蚀及崩塌等外动力地质作用下形成了红色陡崖坡及一系列侵蚀地貌，即丹霞地貌。以龙虎山世界地质公园核心景区仙水岩为例，用面积高程积分方法对江西省丹霞地貌的演化阶段及其主控因素进行了分析。仙水岩景区地层出露一致，丹霞地貌整体处于老年早期的残丘阶段，地貌侵蚀程度较强；由于水系溯源侵蚀，景区内不同部位地貌的演化阶段、类型及面积高程积分值（HI值）不尽相同。本文对江西省丹霞地貌基本特征及控制因素的分析和总结研究将加深对各类丹霞地貌成因的理解，推动丹霞地貌国际化进程，也为其他湿润气候区丹霞地貌地质遗迹的合理利用提供参考。  相似文献   

MM5模式显式微物理方案的对比分析   总被引：15，自引：9，他引：15  

楼小凤周秀骥  胡志晋王鹏云 史月琴 《气象科技》2004,32(1):6-12

介绍了MM5中的显式云物理方案，详细分析了Goddard,Reisner和Schultz方案的物理过程特点和存在的不足。这些云物理方案的多个微物理过程的描述不是很合理，对粒子的自动转化过程都采用阚值，且对雪、霰和雨的数浓度只进行诊断计算。Reisner方案的物理过程相对全面，预报量也较多，但仍存在一定的不足。通过对1992年Andrew台风个例的模拟，发现尽管Reisner方案的物理过程比Goddard和Schultz方案全面，但模拟的台风眼最低气压和地面最大风速并没有优势。所以单一物理过程描述的改善不一定立即带来模式预报成效的提高，因为预报能力取决于整个模式系统的科技水平以及各子程序之间的匹配。  相似文献   

Effects of spatially variable ground motions on the seismic response of a skewed, multi-span, RC highway bridge   总被引：4，自引：0，他引：4  

L. Lou  A. Zerva   《Soil Dynamics and Earthquake Engineering》2005,25(7-10):729-740

This paper presents a study of the influence of spatially variable ground motions on the longitudinal seismic response of a short, three-span, 30-degree skewed, reinforced concrete highway bridge. Linear and nonlinear finite element models are created for the bridge and linear elastic and nonlinear inelastic time history analyses conducted. Three different types of illustrative excitations are considered: The first utilizes spatially variable ground motions incorporating the effects of variable soil conditions, loss of coherency and wave passage as input motions at the structures' supports. The time history with the smallest peak displacement and the one with the largest peak displacement from the spatially variable ones are then used as uniform input motions at all bridge supports. The comparative analysis of the bridge model shows that the uniform ground motion input with the largest peak displacement cannot provide conservative seismic demands for all structural components—in a number of cases it results in lower response than that predicted by spatially variable motions. The present results indicate that there is difficulty in establishing uniform input motions that would have the same effect on the response of bridge models as spatially variable ones. Consequently, spatially variable input motions need to be applied as excitations at the bridge supports.  相似文献   

夏季不同下垫面气象要素的对比分析   总被引：5，自引：4，他引：5  

娄德君李治民  孙卫国 《气象科技》2006,34(2):166-169

对扎龙湿地生态气象站和齐齐哈尔自动气象站2004年6~8月的逐时气温、风速、相对湿度等观测资料进行统计分析,找出了不同下垫面的两站之间不同时次各气象要素的差异,指出两站风速、气温、露点温度、相对湿度、地面温度等的月平均值均存在差异,变化幅度及极值出现时间各有不同;下垫面差异只起到加强或缓和气象要素日变化幅度的作用。所得结果有助于深入了解扎龙湿地的天气变化规律,对未来扎龙湿地气象要素的精细预报以及湿地资源的开发、保护和管理有一定的参考意义。  相似文献   

地震学在减轻矿山地质灾害中的应用进展   总被引：10，自引：1，他引：10  

李世愚  和雪松  张天中  王林瑛  许忠淮  陆其鹄  陈佩燕  沈萍  张少泉  蒋秀琴  潘科  佟晓辉  宋绪友  李铁  金贵杰  左艳  管恩福  孙学会  李国宏  吕毓国 《国际地震动态》2006,(4):1-9

综述了煤矿安全对于地球物理应用的需求,以及近年来地震学在煤矿减轻地质灾害的应用进展,特别是微震监测分析在若干典型煤矿应用得到的初步成果。这些成果不但对于煤矿安全具有重要意义,而且对于认识构造地震成因和验证预测方法,也具有中尺度试验意义。  相似文献   

天然饱水条件下黄铁矿氧化过程的热力学探讨   总被引：1，自引：0，他引：1  

魏有仪  罗健 《矿物岩石》1998,(Z1)

本文从化学热力学角度讨论了黄铁矿在低温低压条件下通过化学作用氧化的历程,指出了决定黄铁矿氧化速率的步骤是黄铁矿的溶解作用,并对一实际水样进行了化学反应的平衡分析  相似文献   

利用声波测井计算岩石的力学参数   总被引：6，自引：0，他引：6       下载免费PDF全文

楼一珊 《探矿工程》1998,(3):47-48

介绍了岩石力学参数的测量方法及岩石动、静弹性参数相关关系,最后用实际声波测井资料来分析计划岩石的力学参数。  相似文献   

Diagenetic reactions in reservoir strata and geochemical properties of pore fluid and its origin in Songliao Basin     

楼章华  蔡希源等 《中国地球化学学报》1998,17(4):346-355

The reservoirs of the SOngliao Basin are composed of typical unstable sandstones,with high percentages of volcanic fragments and feldspar,In the course of sedimentation and burying,a series of physical and chemical reactions took place between minerals and pore water and water-rock reactions and ion exchange caused changes in ion assemblage of pore water,Hydration-hydrolysis,dissolution and the albitization of feldspar made many ions free from their framework and inter into the pore water,and induced the precipitation of a large amount of authigenic minerals such as smectite and chlorite,During the diagenesis of sandstone.diagenetic reactions involved several stages with increasing depth,and so did the precipitation of authigenic minerals and the transformaiton of minerals.The migration of ions is related with the precipitation,transformation and dissolution of authigenic minerals.Thus,to deepen our study on sandstone diagenesis is an important link for the analysis of ion migration in the evolution of pore water ,the origin and evolution of pore water could be tracked in terms of the geochemistry of fluid inclusions in authigenic minerals.And the isotopic composition of the authigenic mineral calcite can provide its genetic information.  相似文献   

Coupled galactic density-wave modes in a composite system of thin stellar and gaseous discs     

Yu-Qing Lou  & Zuhui Fan 《Monthly notices of the Royal Astronomical Society》1998,297(1):84-100

A rotating disc galaxy is modelled as a composite system consisting of thin stellar and gaseous discs, which are described by a two-fluid modal formalism. The composite disc system is assumed to retain axisymmetry in the background equilibrium. General density-wave perturbations in the two discs are coupled through the mutual gravitational interaction. We study the basic properties of open and tight spiral density-wave modes in such a composite disc system. Within the Lindblad resonances, perturbation enhancements of surface mass density in stellar and gaseous discs are in phase; this is also true during the initial growth phase of density-wave perturbations. Outside the Lindblad resonances, there exists a possible spiral density-wave branch for which perturbation enhancements of surface mass density in stellar and gaseous discs are out of phase. We discuss implications of these results on the critical parameters for global star formation in barred and normal spiral galaxies and on magnetohydrodynamic density waves within the Lindblad resonances.  相似文献