新疆西昆仑塔一卡铅-锌矿区成矿特征及找矿方向

塔一卡铅-锌矿区成矿类型具典型的密西西比河谷型层控矿床特征，该矿区的主要含矿地层为下石炭统卡拉巴西塔克组第二岩性段(C1kl^2)白云质灰岩，通过对该矿区成矿特征及控矿条件的分析，指出西昆仑塔卡矿区铅-锌矿勘查的找矿方向。     

MapInfo在矿山生产勘探管理中应用的探讨

根据MapInfo在其它领域应用的原理，利用其包含图形信息对象的数据表是图形和数据之间有机结合的概念，从矿山生产勘探的管理特点出发，论述MapInfo在矿山生产勘探过程中对勘探资料图和储量计算表的对应管理，探讨了矿山生产勘探的管理过程数字化的一种新方法。     

河北兴隆洞子沟银-铜矿床地质特征及成因探讨

根据矿床地质特征、成矿温度、成矿时代及成矿物质来源等方面的研究，认为本矿床成矿流体来源于地慢岩浆水，并有海水混入。成矿物质主要来源于深部地壳和地慢，通过同生断裂喷气—喷流作用，在有利的地层和物理化学条件下沉淀成矿。矿床成因属于同生断裂喷流热液层控矿床。     

内蒙古东部闹牛山铜矿成矿地质背景分析

通过对闹牛山铜矿区与成矿有关的次火山岩岩石化学分析，以及对矿区火山一次火山岩微量元素、稀土元素的分析，结合相关的铅同位素分析，综合分析了该矿床的成矿地质背景。认为：闹牛山铜矿床构造环境属于大陆边缘裂陷带的局部隆起区，成矿火山岩浆为钙碱性，其来源于地壳深部或上地慢，并有上部地壳物质混染。     

红透山矿床变质岩系褶皱构造特征浅析

红透山式铜-锌矿床形成于太古代克拉通裂谷槽盆中海底火山喷发-沉积环境。因此，矿床的空间展布严格受特定的含矿岩系所控制。槽盆构造中的岩层褶皱构造最发育，矿床赋存在具多期褶皱构造叠加的大型同倾向形褶皱内，褶皱的层间虚脱是控矿有利构造空间，可以借此预测矿体侧伏方向及赋存部位。     

大厂矿区坑道磁测找矿试验

大厂矿区一条长1．5km的运输巷道内进行了高精度磁测找矿试验，并进行了地质钻探验证。结果表明：在将局部磁性干扰压抑后，所获相对磁异常是可以取得找矿效果的。     

云南武定迤腊厂铜矿含矿石英脉40 Ar-39Ar年龄及其意义

对武定迤腊厂铜矿成矿期石英进行了40Ar-39Ar同位素年龄测定,得到马鞍形年龄谱,坪年龄为(784.25±0.95)Ma,等时线年龄为(783.93±8.59)Ma.地质特征研究表明该矿床后期改造作用明显,并非同生沉积或成岩作用早期成矿,而与晋宁期Rodina大陆裂解有关.武定迤腊厂铜矿的形成可能是在Rodinia大陆裂解时,从深部带来大量成矿物质,改造成岩时期初始的矿化,形成矿床的叠加富集和最终定位,晋宁-澄江期是该矿床的主成矿期.     

东川桃园式铜矿Ar-Ar同位素年龄及意义

通过对东川桃园铜矿与铜矿共生石英的40Ar/39Ar同位素年龄的测定,得到马鞍形年龄谱,其坪年龄为768.43Ma±0.58Ma,等时线年龄为770.00Ma±5.44Ma。该矿床后期改造作用明显,并非同生沉积或成岩作用早期成矿,而与晋宁期Rodina大陆裂解有关。东川铜矿的形成可能是在Rodinia大陆裂解时,从深部带来大量成矿物质改造成岩时期初始的矿化,形成矿床的叠加富集和最终定位,因此,晋宁-澄江期是东川铜矿的主成矿期。     

采空区上方修建大型建筑物地基稳定性评价

地表移动变形随时间的稳定性及剩余变形问题一直是采动覆岩沉陷研究的重要方面。笔者分析了采动地表移动变形的时间过程,探讨了地表沉陷的延续时间及地表剩余沉陷的预计方法,给出了采空区上方修建大型建筑物地基稳定性评价的指标,对采空区上建设建筑物提出了相应的技术措施。     

Genetic significance of fluid inclusions in the CSA Cu–Pb–Zn deposit, Cobar, Australia

CSA mine exploits a ‘Cobar-type’ Cu–Pb–Zn±Au±Ag deposit within a cleaved and metamorphosed portion of the Cobar Supergroup, central New South Wales. The deposit comprises systems of ‘lenses’ that encompass veins, disseminations and semi-massive to massive Cu–Pb–Zn ores. The systems and contained lenses truncate bedding, are approximately coplanar with regional cleavage and similarly oriented shear zones and plunge parallel to the elongation lineation. Systems have extreme vertical continuity (>1000 m), short strike length (400 m) and narrow width (100 m), exhibit vertical and lateral ore-type variation and have alteration haloes. Models of ore formation include classical hydrothermalism, structurally controlled remobilisation and polymodal concepts; syntectonic emplacement now holds sway.Fluid inclusions were examined from quartz±sulphide veins adjacent to now-extracted ore, from coexisting quartz–sulphide within ore, and from vughs in barren quartz veins. Lack of early primary inclusions precluded direct determination of fluids associated with D₂–D₃ ore and vein emplacement. Similarly, decrepitation (by near-isobaric heating) of the two oldest secondary populations precluded direct determination of fluid phases immediately following D₂–D₃ ore and vein emplacement. Post-decrepitation outflow (late D₃ to early post-D₃) is recorded by monophase CH₄ inclusions. Entrained outflow of deeply circulated meteoric fluid modified the CH₄ system; modification is recorded by H₂O+CH₄ and H₂O+(trace CH₄) secondary populations and by an H₂O+(trace CH₄) primary population. The contractional tectonics (D₂–D₃) of ore emplacement was superseded by relaxational tectonics (D_4P) that facilitated meteoric water penetration and return flow.Under D₂ prograde metamorphism, entrapment temperatures (Tt) and pressures (Pt) for pre-decrepitation secondary inclusions are estimated as Tt300–330 °C and Pt1.5–2 kbar≈Plith (the lithostatic pressure). Decrepitation accompanied peak metamorphism (T350–380 °C) in mid- to late-D₃, while in late-D₃ to early post-D₃, essentially monophase CH₄ secondary inclusions were entrapped at Tt350 °C and Pt=1.5–2 kbar≈Plith. Subsequently, abundant CH₄ and entrained meteoric water were entrapped as H₂O+CH₄ secondaries under slowly decreasing temperature (Tt330–350 °C) and constant pressure (Pt1.5–2 kbar). Finally, with increasingly dominant meteoric outflow, H₂O+(trace CH₄) populations record decreasing temperatures (Tt>300 to <350 down to 275–300 °C) at pressures of Phydrostatic<Pt (1 kbar) <Plith (1.5 kbar).The populations of inclusions provide insight into fluid types, flow regimes and P–T conditions during parts of the deposit's evolution. They indirectly support the role of basin-derived CH₄ fluids in ore formation, but provide no insight into a basement-sourced ore-forming fluid. They fully support post-ore involvement of meteoric water. The poorly constrained entrapment history is believed to span 10 Ma from 395 to 385 Ma.