浅谈延吉水洞地区的寻找金矿前景

水洞地区位于吉林省东部,处于天山—兴安地槽褶皱区,吉黑褶皱系延边优地槽褶皱带内,是我国比较重要的金成矿带之一[1]。本文介绍了该区的地层、构造、岩浆岩情况。通过化探分析确定了Au元素异常范围,且物探异常区与相应的化探范围内蚀变带相吻合,为该区寻找浅成中、低温热液型金矿奠定了基础。根据野外勘查工作中的实际情况对该区的找矿前景进行预测。     

钦-杭结合带在中生代构造转折事件以前的板块构造机制

钦州湾—杭州湾结合带是位于扬子与华夏两大古陆块中间的巨型构造结合带,在演化成西太平洋活动大陆边缘之前,经历了多期次的构造-岩浆事件。扬子和华夏板块于新元古代通过四堡造山运动(1 000~880 Ma)沿江山—绍兴断裂,经赣东北、湘中至钦州湾地区发生碰撞-拼合事件,拼合界线大致位于钦州湾—杭州湾结合带内,形成"两陆夹一盆"的主要格局。后碰撞过程经历了造山后岩浆活动和大陆拉张裂解两个过程,在结合带形成广阔的拉张盆地,加里东期(460~410 Ma)以及印支期(250~200 Ma)发生的碰撞-拼合事件导致扬子和华夏地块多次再造,引发强烈的构造-岩浆活动,并形成了华南统一的沉积环境。受西太平洋板块俯冲影响,华南地区中生代构造转折事件(125~140 Ma)使华南地区主要构造背景由碰撞挤压调整为岩石圈减薄,成为华南最重要的岩浆活动和成矿期。根据内部结构的不均一性和演化历史差异,钦州湾—杭州湾结合带可分为北段、中段和南段3段。其中,中段与传统南岭大体一致;北段为南岭以北地区,即绍兴—江山—萍乡一带;南段为南岭以南地区,大致与云开隆起—十万大山盆地相当。年代学和地球化学研究显示,在云开地块西缘的一系列变质基性岩、超基性岩和变质基性火山岩形成于新元古代洋中脊(MORB)或者岛弧(ITA)特征的构造环境,最近在岑溪一带发现形成于加里东期(441 Ma)的变质火山岩同样具有MORB型地球化学特征。在十万大山两侧发现早中生代的酸性火山岩和流纹岩具有典型岛弧型火山岩地球化学特征。可见结合带南段曾经存在古老洋壳,先后经历了新元古代、加里东期和印支期的碰撞造山事件,与北段演化历史具有一致性。     

钦-杭成矿带主要金属矿床成矿系列

钦-杭成矿带是华南地区最重要的Cu-Pb-Zn-Au、W-Sn-Bi-Mo和Fe-Mn-S多金属成矿带。在前人工作基础上,根据矿床的成因组合、形成构造环境及其随地质历史演化的特点,将钦-杭成矿带主要金属矿床归纳为中新元古代海底喷流沉积型铜多金属矿床、新元古代海相沉积-变质型铁锰矿床、古生代海相沉积-叠生改造型铜铅锌铁锰矿床、加里东期与花岗岩类有关的钨钼金银多金属矿床、印支期与花岗岩类有关的钨锡铌钽铀多金属矿床、燕山期与花岗岩类有关的铜铅锌金钨锡多金属矿床、与区域动力变质热液作用有关的金银矿床等7个矿床成矿系列。进而讨论了各成矿系列的主要矿床类型、矿床地质特征和时空分布规律,初步认为,中新元古代海底喷流沉积型块状硫化物铜多金属矿床与大陆边缘岛弧火山作用有关,主要分布于扬子陆块东南缘和华夏陆块西北缘古岛弧褶皱区;新元古代受变质铁锰矿床与大陆裂谷火山作用有关,并经受了后期区域变质、热变质作用的改造,主要分布于加里东期隆起区;古生代层控型铜铅锌铁锰矿床与海底热水沉积成矿作用有关,且不同程度地受到后期岩浆-热液活动的叠加改造,主要分布于海西—印支期坳陷区与隆起区的过渡部位;加里东期斑岩-夕卡岩-热液脉型钨钼金银多金属矿床与奥陶纪末—志留纪陆内造山作用有关,主要分布于加里东期隆起区;印支期斑岩-夕卡岩-热液脉型钨锡铌钽铀多金属矿床与印支板块向华南板块的俯冲碰撞有关,成矿作用发生在后碰撞伸展阶段,主要分布于海西—印支期隆起区边缘;燕山期斑岩-夕卡岩-热液脉型铜铅锌金钨锡多金属矿床与岩石圈伸展引起的玄武岩底侵作用有关,广泛分布于海西—印支期拗陷区或中生代盆地边缘;与区域动力变质热液作用有关的金银矿床成矿系列,与印支—燕山期大规模的逆冲推覆作用有关,主要发育于钦-杭结合带两侧古陆边缘。     

卵石地层的特殊性及其对基坑支护的影响分析

主要从卵石地层的特征分类、特殊结构及场内施工条件3个方面,对基坑支护结构选型及施工工艺选择进行深入、系统的分析论证,力求使在卵石地层中的基坑支护设计方案更科学、经济,使施工方法、工艺更具可操作性。     

Kinematics of syn-tectonic unconformities and implications for the tectonic evolution of the Hala'alat Mountains at the northwestern margin of the Junggar Basin,Central Asian Orogenic Belt

The Hala’alat Mountains are located at the transition between the West Junggar and the Junggar Basin.In this area,rocks are Carboniferous,with younger strata above them that have been identified through well data and high-resolution 3D seismic profiles.Among these strata,seven unconformities are observed and distributed at the bases of:the Permian Jiamuhe Formation,the Permian Fengcheng Formation,the Triassic Baikouquan Formation,the Jurassic Badaowan Formation,the Jurassic Xishanyao Formation,the Cretaceous Tugulu Group and the Paleogene.On the basis of balanced sections,these unconformities are determined to have been formed by erosion of uplifts or rotated fault blocks primarily during the Mesozoic and Cenozoic.In conjunction with the currently understood tectonic background of the surrounding areas,the following conclusions are proposed:the unconformities at the bases of the Permian Jiamuhe and Fengcheng formations are most likely related to the subduction and closure of the Junggar Ocean during the late Carboniferous-early Permian;the unconformities at the bases of the Triassic Baikouquan and Jurassic Badaowan formations are closely related to the late Permian-Triassic Durbut sinistral slip fault;the unconformities at the bases of the middle Jurassic Xishanyao Formation and Cretaceous Tugulu Group may be related to reactivation of the Durbut dextral slip fault in the late Jurassic-early Cretaceous,and the unconformity that gives rise to the widely observed absence of the upper Cretaceous in the northern Junggar Basin may be closely related to large scale uplift.All of these geological phenomena indicate that the West Junggar was not calm in the Mesozoic and Cenozoic and that it experienced at least four periods of tectonic movement.     

一种亮星识别算法及其在天文定向中的应用

基于全站仪对任意亮星的观测采样,提出了一种利用高度角序列和水平角速率进行联合匹配的任意亮星识别算法。通过引入天体地平坐标计算程序,算法可正确辨别行星和恒星。本文分析了任意亮星高度角和水平角速率的观测误差和计算误差,以此给出了匹配阈值条件的设定依据,并在此基础上制定了有效的匹配策略。仿真计算及实际观测试验均表明,该算法具有100%的识别成功率,远优于现有算法。将此算法应用于任意亮星天文定向,定向结果的内符合精度达到2″,外部检核精度达到1.6″。采用多颗任意亮星进行定向,可有效减弱由测站位置误差引入的定向系统误差,提高绝对定向精度。本文提出的天文定向适用于多云及雾霾天气。     

西藏冈底斯成矿带矿化蚀变提取与成矿分析——以尼玛县帮勒地区为例

冈底斯成矿带是我国极具找矿潜力的地带,但受自然条件限制,该地带矿产资源开发程度普遍偏低。选取冈底斯成矿带北部尼玛县帮勒地区为研究区,以Landsat-8OLI数据为主要信息源,采用主成分分析法提取研究区铁染和羟基矿化蚀变信息。在GIS平台上,将提取的蚀变信息结合研究区现有地质、化探、矿产等资料进行综合分析,依据成矿理论,圈定2个成矿远景区。经野外验证,文中获取的矿化蚀变信息分布状况与已知矿点和已探明蚀变带的空间一致性高。矿化蚀变带的探明能够为区域矿产资源开发与勘查提供帮助。     

中国锡矿成矿规律概要

我国锡矿资源丰富,矿床类型比较齐全。在锡矿资源储量中占有较大比重的主要是锡石—硫化物型、矽卡岩型和石英脉型;从开采和利用角度来说,最为重要的是锡石—硫化物型和石英脉型。锡石—硫化物型主要集中在桂北、滇东等地,矽卡岩型集中分布在南岭中段湘南等矿集区、石英脉型则主要集中在华南地区的闽西、赣中、粤北、湘南等地;成矿时代以中生代最为重要;成矿大地构造背景以造山运动之后的大陆环境为主,构造变动剧烈,深大断裂纵横交错,岩浆活动频繁,特别是与锡成矿作用关系密切的中生代花岗岩类非常发育,最具特色。本次在对全国873处锡矿矿产地资料进行系统梳理的基础上,深入总结了全国锡矿的成矿规律,厘定出20个以锡为主或锡较为重要的矿床成矿系列,认为锡石—硫化物型、矽卡岩(—云英岩型)、石英脉型和岩体型4类锡矿类型,应该作为重点预测类型,并划分出44个成锡带,提出了19个重要工作部署区,并编制了中国成锡带图、中国锡矿成矿规律图等系列图件,为潜力评价预测工作提供了理论依据。     

三江造山带义敦岛弧中段格聂（南）花岗岩体地球化学特征及地质意义

夹持于甘孜—理塘结合带与金沙江结合带之间的义敦弧岩浆岩带上发育了3条纵贯南北的造山花岗岩带,其中:中带形成了由20余个岩体组成的雀而山—格聂花岗岩带和相关的银、锌、铅-锌多金属矿床。本文对格聂(南)花岗岩体进行研究,发现其岩石类型为花岗闪长岩、二长花岗岩和钾长花岗岩三类,以二长花岗岩为主体。锆石LA-ICP-MS U-Pb定年结果表明格聂花岗岩的成岩年龄为89.9±3.6Ma。地球化学研究表明,岩石中主量元素化学成分具有富硅、富铝、低钠高钾的特征,为典型的S型花岗岩。铝饱和指数ASI1,指示岩浆源自地壳;(CaO)%/(Na2O)%值等于0.1左右,表明源岩为大陆地壳沉积岩区的泥质岩。稀土总量均值228.83×10-6,稀土配分曲线呈略右倾近直线海鸥型,与地壳熔融型花岗岩形态一致。轻重稀土分馏不明显;铕出现明显负异常(δEu=0.13),显示岩浆分异结晶作用强烈。微量元素蛛网图上明显亏损大离子亲石元素Sr;富集高场强元素U。Rb/Sr平均比值14.97,表明格聂花岗岩的源岩为上部陆壳。结合Rb-(Y+Nb)图解、(Rb/30)-Hf-(Ta×3)图解、R1-R2变异图解,格聂南岩体形成于后碰撞造山环境,应是甘孜-理塘洋盆和金沙江洋盆闭合后,造山后伸展作用活动的产物。     

White mica K–Ar geochronology of Sanbagawa eclogites from Southwest Japan: implications for deformation-controlled K–Ar closure temperature

White mica (phengite and paragonite) K–Ar ages of eclogite-facies Sanbagawa metamorphic rocks (15 eclogitic rocks and eight associated pelitic schists) from four different localities yielded ages of 84–89 Ma (Seba, central Shikoku), 78–80 Ma (Nishi-Iratsu, central Shikoku), 123 and 136 Ma (Gongen, central Shikoku), and 82–88 Ma (Kotsu/Bizan, eastern Shikoku). With the exception of a quartz-rich kyanite-bearing eclogite from Gongen, white mica ages overlap with the previously known range of phengite K–Ar ages of pelitic schists of the Sanbagawa metamorphic belt and can be distinguished from those of the Shimanto metamorphic belt. The similarity of K–Ar ages between the eclogites and surrounding pelitic schists supports a geological setting wherein the eclogites experienced intense ductile deformation with pelitic schists during exhumation. In contrast, phengite extracted from the Gongen eclogite, which is less overprinted by a ductile shear deformation during exhumation, yielded significantly older ages. Given that the Gongen eclogite is enclosed by the Higashi-Akaishi meta-peridotite body, these K–Ar ages are attributed to excess ⁴⁰Ar gained during an interaction between the eclogite and host meta-peridotite with mantle-derived noble gas (very high ⁴⁰Ar/³⁶Ar ratio) at eclogite-facies depth. Fluid exchange between deep-subducted sediments and mantle material might have enhanced the gain of mantle-derived extreme ⁴⁰Ar in the meta-sediment. Although dynamic recrystallization of white mica can reset the Ar isotope system, limited-argon-depletion due to lesser degrees of ductile shear deformation of the Gongen eclogite might have prevented complete release of the trapped excess argon from phengites. This observation supports a model of deformation-controlled K–Ar closure temperature.