四川理塘如金沟铜矿区矿化特征初探

这里主要从成矿地质背景、控矿构造、赋矿火山岩分布、矿床特征等宏观地质现象,结合岩矿石结构的构造与成份等微观特征的深入研究,首次确定了如金沟铜矿区赋矿次火山岩的存在.初步认为其主导矿床成因类型为次火山岩型,在矿区内形成次火山岩型→火山热液型→构造热液型较完整的矿化分带系列.     

Diamond in Oceanic Peridotites and Chromitites: Evidence for Deep Recycled Mantle in the Global Ophiolite Record

Diamonds have been discovered in mantle peridotites and chromitites of six ophiolitic massifs along the 1300 km‐long Yarlung‐Zangbo suture (Bai et al., 1993; Yang et al., 2014; Xu et al., 2015), and in the Dongqiao and Dingqing mantle peridotites of the Bangong‐Nujiang suture in the eastern Tethyan zone (Robinson et al., 2004; Xiong et al., 2018). Recently, in‐situ diamond, coesite and other UHP mineral have also been reported in the Nidar ophiolite of the western Yarlung‐Zangbo suture (Das et al., 2015, 2017). The above‐mentioned diamond‐bearing ophiolites represent remnants of the eastern Mesozoic Tethyan oceanic lithosphere. New publications show that diamonds also occur in chromitites in the Pozanti‐Karsanti ophiolite of Turkey, and in the Mirdita ophiolite of Albania in the western Tethyan zone (Lian et al., 2017; Xiong et al., 2017; Wu et al., 2018). Similar diamonds and associated minerals have also reported from Paleozoic ophiolitic chromitites of Central Asian Orogenic Belt of China and the Ray‐Iz ophiolite in the Polar Urals, Russia (Yang et al., 2015a, b; Tian et al., 2015; Huang et al, 2015). Importantly, in‐situ diamonds have been recovered in chromitites of both the Luobusa ophiolite in Tbet and the Ray‐Iz ophiolite in Russia (Yang et al., 2014, 2015a). The extensive occurrences of such ultra‐high pressure (UHP) minerals in many ophiolites suggest formation by similar geological events in different oceans and orogenic belts of different ages. Compared to diamonds from kimberlites and UHP metamorphic belts, micro‐diamonds from ophiolites present a new occurrence of diamond that requires significantly different physical and chemical conditions of formation in Earth's mantle. The forms of chromite and qingsongites (BN) indicate that ophiolitic chromitite may form at depths of >150‐380 km or even deeper in the mantle (Yang et al., 2007; Dobrthinetskaya et al., 2009). The very light C isotope composition (δ13C ‐18 to ‐28‰) of these ophiolitic diamonds and their Mn‐bearing mineral inclusions, as well as coesite and clinopyroxene lamallae in chromite grains all indicate recycling of ancient continental or oceanic crustal materials into the deep mantle (>300 km) or down to the mantle transition zone via subduction (Yang et al., 2014, 2015a; Robinson et al., 2015; Moe et al., 2018). These new observations and new data strongly suggest that micro‐diamonds and their host podiform chromitite may have formed near the transition zone in the deep mantle, and that they were then transported upward into shallow mantle depths by convection processes. The in‐situ occurrence of micro‐diamonds has been well‐demonstrated by different groups of international researchers, along with other UHP minerals in podiform chromitites and ophiolitic peridotites clearly indicate their deep mantle origin and effectively address questions of possible contamination during sample processing and analytical work. The widespread occurrence of ophiolite‐hosted diamonds and associated UHP mineral groups suggests that they may be a common feature of in‐situ oceanic mantle. The fundamental scientific question to address here is how and where these micro‐diamonds and UHP minerals first crystallized, how they were incorporated into ophiolitic chromitites and peridotites and how they were preserved during transport to the surface. Thus, diamonds and UHP minerals in ophiolites have raised new scientific problems and opened a new window for geologists to study recycling from crust to deep mantle and back to the surface.     

南雄断裂带构造演化及铀成矿作用

文章从粤北地区受南雄断裂带控制的南东侧盆地沉积建造组合、构造岩成分特征等入手,探讨南雄断裂带的发生发展、构造动力演化及不同阶段断裂组合形式和铀矿床区域定位规律,提出与南雄断裂带强烈挤压阶段相配套的北西向张性断裂系统是幔源岩浆作用及其深部热流体侵入通道和铀矿体赋存部位的观点。下一步工作重点应针对北西向张性断裂的隐蔽性特点,选择有效的地球物理和地球化学勘查手段,查明北西向断裂地表出露的确切位置、产状变化及其空间展布规律,配合钻探工程揭露验证,不断深化对区域铀成矿规律的认识,扩大找矿效果。     

南秦岭佛坪隆起的成因探讨——构造解析的证据

通过对佛坪隆起基底及其周围地区构造面理和线理的系统测量和统计,恢复其古应力场,揭示区域构造应力场的分布规律,进而探讨佛坪隆起的成因机制。研究结果表明,佛坪隆起主体及其北部龙草坪隆起区外围地层中的构造片理呈外倾的封闭环状展布,结合古构造应力场分析,证明佛坪基底抬升主要生成于穹状隆起,这种穹状隆升与该区岩浆侵入活动密切相关。综合区域构造解析与古应力场分析表明,佛坪穹隆是在早期近垂向的穹状隆升的基础上,叠加了后期南北向挤压构造才奠定了其基本构造面貌。     

常州市区地下水污染研究

根据常州市地下水环境背景值、水质长期监测数据,分析常州市地下水水质演变规律。通过分析1982年至2009年水质状况,对地下水污染程度进行分级,综合评价地下水水质。并结合地下水污染因子变化规律、水化学类型变化趋势,提出地下水保护综合治理措施。     

辽东中生代晚期和古近纪玄武岩及深源捕虏晶--对岩石圈地幔性质的制约

辽东地区玄武岩的K-Ar定年结果表明,曲家屯玄武岩形成于晚白垩世,K-Ar年龄为81．58±2．46Ma;乱石山子玄武岩形成于古近纪,K-Ar年龄为58．36±1．64Ma。本区玄武岩含有丰富的橄榄石、单斜辉石和角闪石捕虏晶。乱石山子玄武岩中橄榄石捕虏晶的Mg^#值（79．5-88．5之间,平均值为84）较曲家屯玄武岩中橄榄石捕虏晶Mg^#值（77．0～79．8之间,平均值为78．4）偏高;单斜辉石捕虏晶为透辉石,其从核部到边部的Mg^#等变化趋势与橄榄石类似;斜方辉石捕虏晶为占铜辉石,其Mg^#值介于85．2-87．6之间,平均值为86．4。捕虏晶发育的环状裂隙、扭折带、矿物成分环带以及捕虏晶与主岩Mg^#值之间的不平衡均暗示它们为玄武质岩浆上升捕获的早期岩浆晶出矿物的堆晶体。玄武岩的岩石地球化学分析结果表明：（1）它们属于碱性系列,为碱性玄武岩,曲家屯玄武岩较乱石山子玄武岩贫硅、镁,富钙、铝,它们均具有原始岩浆的特征;（2）二者具有相似的稀土元素配分模式,但曲家屯玄武岩轻稀土元素总量更高,且轻重稀土元素分离程度高;（3）二者具有相似的Sr-Nd同位素组成,Isr和εNd（t）值分别介于0．7039～0．7045和＋1．60～＋3．69,反映了亏损的岩石圈地幔特征。     

地震勘探在东兴盐矿的应用

在安徽定远东兴盐矿勘探中,通过采用地震反射波法与钻孔的对比分析,充分说明地震反射波法在第三系地层中寻找石膏矿、岩盐等沉积型矿藏有着良好的应用前景。     

水稻土中重金属元素Cd、Pb的竞争吸附——以长株潭地区水稻土为例

对中国南方的3个水稻土样品进行了Cd、Pb单一离子和混合离子吸附特点的研究。结果表明,3个水稻土样品中Cd、Pb的吸附特点都相似,Langmuir等温方程可很好地描述Cd、Pb的吸附等温线。3个土壤样品中,有较高pH值和较低有机物、CEC浓度、粘土含量、高岭石含量的2个土壤样品对Cd、Pb有较大的吸附量,且其等温吸附拟合的最大吸附量（B）也较大。在两组分混合溶液中,尽管共存离子的存在影响了土壤对单一离子的吸附,同时土壤对Cd的吸附在一定程度上受影响的程度大,但3个土壤样品都表现出对Pb有强的吸附能力。在3个土壤样品中,Langmuir等温方程中Pb的健合能常数（K）都大于Cd的健合能常数（K）,混合溶液中的K值高于单一溶液的K值,表明2种金属离子对吸附位点的竞争提高了特定吸附位点的保持力,使金属离子在土壤中特定位点的吸附更加坚固。     

浙东白垩纪北漳和梁弄花岗岩体及其暗色岩石包体研究

浙东地区晚中生代花岗岩类在岩性上分为三类：花岗岩-二长花岗岩、钾长花岗岩和A型花岗岩。对后两类花岗岩已有较多研究,但对前一类,尤其是二长花岗岩的研究还较薄弱。选择浙东具代表性的北漳和梁弄二长花岗岩体及其所含暗色岩石包体,以及共生的石英闪长岩类,通过系统的岩石学与地球化学对比研究,提出浙东二长花岗岩属准铝质、高钾钙碱性Ⅰ型花岗岩类演化系列,暗色岩石包体是由花岗质岩浆在深部析离出的镁铁质微粒包体(MME),成分特征类似于石英闪长岩,说明三者具内在成因联系,均与俯冲作用关系密切。     

湘西沃溪钨锑金矿床成矿的独特性

沃溪钨锑金矿床位于NE向雪峰弧形构造带向北西凸出的转折部位东段,赋存于新元古界板溪群马底驿组紫红色板岩中,产在沃溪近EW向低角度拆离断层下盘沿层发育的层间剪切断裂系统,以层间石英脉型矿体为主,矿化作用在时间上和空间上具有一定的分带性和规律性.矿体沿倾向延深大于走向延长数倍至10余倍,并普遍存在侧伏延伸的规律.杂多酸络合物作为W,Sb,Au成矿组合的共同载体,使它们共同进入热液地球化学迁移,并生成钨锑金共生组合的金矿床,成为重要的成矿地球化学机制.