大庙式铁矿的找矿远景和方向     

赵桂秋  纪广俭  刘小滨 《吉林地质》2012,(3):53-56,130

大庙式铁矿的成矿和找矿远景有两个方面,其一是在大庙岩体的内部,其二是在岩体之外的尚义—平泉断裂带沿线的深部。根据岩体的地表形态呈南宽北窄的似三角形,且南部边界平直并有平行的断层,推测岩体是由主侵体和溢流体组成的直立状勾手形综合体,南面相当直立的手掌,构成主侵体,北面相当于平放的并拢五指,组成溢流体。由于南面的主侵体可以一直向下延深,具有很大深度,有充足成矿物质来源,因而具有很大的成矿和赋矿远景,是找矿的重点部位。在大庙岩体的外围,沿尚义—平泉大断裂带两侧,西起崇礼,东到平泉200多千米长的地段内,有众多基性、超基性岩体发育,其内有较多的富磁铁矿岩石,构成超贫级铁矿,这些基性、超基性岩体可能属于隐伏在深部的大型基性、超基性岩体的浅部标志,具有较大的成矿和找矿远景。  相似文献   

甘肃北山地区黑山铜镍矿化基性—超基性杂岩体SHRIMP锆石U-Pb定年及其地质意义   总被引：1，自引：0，他引：1  

杨建国  王磊  王小红  谢燮  齐正广 《中国区域地质》2012,(2):448-454

黑山铜镍矿床位于塔里木板块东北部的北山裂谷带内,庙庙井-双鹰山深大断裂南侧,含矿基性—超基性复式杂岩体侵位于青白口系大豁落山组和寒武系双鹰山组中。矿化主要赋存于杂岩体内的橄榄岩和角闪辉长岩内。采用锆石离子探针微区原位（SHRIMP）法获得矿化角闪辉长岩中锆石的U-Pb年龄为374.6Ma±5.2Ma,表明该含矿杂岩体的侵位及矿化作用均发生于晚泥盆世。这一年龄数据的获得不仅对重新认识北山地区的地质构造演化具有重要意义,而且为北山地区开展铜镍矿找矿提出了新方向。  相似文献   

Effects of low-viscous layers and a non-zero obliquity on surface stresses induced by diurnal tides and non-synchronous rotation: The case of Europa     

Hermes M. Jara-Orué  Bert L.A. Vermeersen 《Icarus》2011,215(1):417-438

In this study we present a semi-analytical Maxwell-viscoelastic model of the variable tidal stress field acting on Europa’s surface. In our analysis, we take into account surface stresses induced by the small eccentricity of Europa’s orbit, the non-zero obliquity of Europa’s spin axis - both acting on a diurnal 3.55-days timescale - and the reorientation of the ice shell as a result of non-synchronous rotation (NSR). We assume that Europa’s putative ocean is covered by an ice shell, which we subdivide in a low-viscous and warm lower ice layer (asthenosphere, viscosity 10¹²-10¹⁷ Pa s), and a high-viscous and cold upper ice layer (lithosphere, viscosity 10²¹ Pa s).Viscoelastic relaxation influences surface stresses in two ways: (1) through viscoelastic relaxation in the lithosphere and (2) through the viscoelastic tidal response of Europa’s interior. The amount of relaxation in the lithosphere is proportional to the ratio between the period of the forcing mechanism and the Maxwell time of the high-viscous lithosphere. As a result, this effect is only relevant to surface stresses caused by the slow NSR mechanism. On the other hand, the importance of the viscoelastic response on surface stresses is proportional to the ratio between the relaxation time (τ_j) of a given viscoelastic mode j and the period of the forcing function. On a diurnal timescale the fast relaxation of transient modes related to the low viscosity of the asthenosphere can alter the magnitude and phase shift of the diurnal stress field at Europa’s surface. The effects are largest, up to 20% in magnitude and 7° in phase for ice rigidities lower than 3.487 GPa, when the relaxation time of the aforementioned transient modes approaches the inverse of the average angular rate of Europa’s orbit. On timescales relevant for NSR (>10⁴ years) the magnitude and phase shift of NSR surface stresses can be affected by viscoelastic relaxation of the ocean-ice boundary. This effect, however, becomes only important when the behavior of the lithosphere w.r.t. NSR approaches the fluid limit, i.e. for strong relaxation in the lithosphere. The combination of NSR and diurnal stresses for different amounts of viscoelastic relaxation of NSR stresses in the lithosphere leads to a large variety of global stress fields that can explain the formation of the large diversity of lineament morphologies observed on Europa’s surface. Variation of the amount of relaxation in the lithosphere is likely due to changes in the spin rate of Europa and/or the rheological properties of the surface.In addition, we show that a small obliquity(<1°) can have a considerable effect on Europa’s diurnal stress field. A non-zero obliquity breaks the symmetric distribution of stress patterns with respect to the equator, thereby affecting the magnitude and orientation of the principal stresses at the surface. As expected, increasing the value of Europa’s obliquity leads to larger diurnal stresses at the surface, especially when Europa is located 90° away from the nodes formed by the intersection of its orbital and equatorial planes.  相似文献   

Brachinite meteorites: Partial melt residues from an FeO-rich asteroid     

《Chemie der Erde / Geochemistry》2014,74(3):311-329

Brachinites are ultramafic, dunitic to wherlitic, unbrecciated and essentially unshocked rocks that are low in SiO₂ (∼36–39 wt.%), high in MgO (∼27–30 wt.%) and notably high in FeO (∼26–37 wt.%), and low in Al₂O₃ (∼0.2–2.5 wt.%) and combined alkalis Na₂O and K₂O (∼0–0.7 wt.%). They consist mostly of olivine (∼71–96 vol.%; ∼Fo_64–73), major clinopyroxene (minor to ∼15 vol.%; ∼En_40–63Wo_36–48), with variable small amounts of plagioclase (0 to ∼10 vol.%; ∼An_15–33), and minor to trace amounts of orthopyroxene (none to ∼20 vol.%; En_69–73Wo_2–4), Fe-sulfides (trace to ∼7 vol.%), chromite (none to ∼5 vol.%), phosphates (none to ∼3 vol.%) and metallic Fe,Ni (trace to ∼2 vol.%). Minerals tend to be homogeneous, and textures are medium to coarse-grained (∼0.1–1.5 mm), with olivine commonly displaying triple junctions. Brachina has near-chondritic lithophile element abundances, whereas other brachinites show variable depletions in Al, Ca, Rb, K, Na, and LREE. Siderophile element abundance patterns vary and range from ∼0.01 to ∼0.9 CI. Oxygen isotope composition (Δ¹⁷O) ranges from ∼−0.09 to −0.39‰, with the mean = −0.23 ± 0.14‰. Brachinites are ancient rocks, as was recognized early by the detection, in some brachinites, of excess ¹²⁹Xe from the decay of short-lived ¹²⁹I (half-life 17 Ma) and of fission tracks from the decay of ²⁴⁴Pu (half-life 82 Ma) in phosphate, high-Ca clinopyroxene and olivine. The first precise crystallization age was determined for Brachina using ⁵³Mn–⁵³Cr systematics, relative to the Pb–Pb age of the angrite LEW 86010, and yielded an age of 4563.7 ± 0.9 Ma. Thus, Brachina is at most ∼4 Ma younger that the CAIs whose age is 4567.2 ± 0.6 Ma. There is no consensus on the origin of brachinites, but they most likely are primitive achondrites, i.e., ultra-mafic residues from various low degrees of partial melting. Partial melting experiments suggest that they possibly formed from a parent lithology chemically similar but not identical to the Rumuruti (R) chondrites, although the different oxygen isotopic compositions of the R chondrites and the brachinites put a serious constraint on this hypothesis. The apparent lack of abundant rocks representing the partial melts suggests that brachinites may have formed on a parent body <∼100 km in radius, where early partial melts were removed from the parent body by explosive pyroclastic volcanism. Graves Nunataks 06128 and 06129 are felsic, andesitic basalts which have properties that suggest a relationship to brachinites and thus, may be samples of the elusive partial melts.  相似文献   

用控矿断裂数字模拟预测小秦岭东桐峪Q8号脉的深部矿体     

邢俊兵 《地质与勘探》2014,50(Z1):1299-1303

脉状矿床是我国重要的一类矿床,矿体普遍受断裂构造控制。我国早期对矿床的勘探深度较浅,岩体深部是继续找矿的方向。前人已研究出一种脉状矿床深部矿体定位预测的方法—控矿断裂数字模拟法,并编制了相应的软件：控矿断裂模拟找矿预测系统。它通过研究断裂波形、断裂运动对矿体位置的控制规律,对脉状矿体进行深部预测。我们运用该方法对小秦岭东桐峪Q8号脉进行深部预测,取得了较好效果。  相似文献   

栅格DEM坡体因子融合方法北大核心CSCD     

周访滨  谢财昌  王俊  陈百了  胡奕 《测绘通报》2022,(8):104-109

坡体是自然地形实体的基本组成单元,利用综合性坡体因子分析和挖掘地形隐含信息,有助于区域地形地貌分析及规划利用。本文针对当前坡体综合表达因子(LS)未顾及坡宽因子的缺陷,采用归一化几何运算法将坡长(L)、坡度(S)、坡宽(W)进行融合,获取了一种新的坡体融合因子LSW。以DEM为数据源、黄土高原某小流域局部范围为典型研究区,在提取L、S、W及LS因子的基础上,分别以L×S×W、L+S+W、LS×W及LS+W共4种方式进行融合试验。结果表明,L+S+W融合方式获取的坡体LSW因子标准差矩阵均值最小,为0.234 4,有效平衡了各单地形因子对融合坡体因子LSW的贡献度,信息熵值计算分析也实证了L+S+W融合方式具有最优性。  相似文献   

碧玺自发极化效应的环境应用以及人体保健作用     

李琳  传秀云 《岩石矿物学杂志》2014,33(S2):177-184

碧玺是一种色彩丰富倍受青睐的宝石,同时也可以作为环境矿物用来治理环境.碧玺具独特的自发极化现象,具有表面电场,可以电解水、吸附带电离子、释放空气负离子.这些独特的性质赋予碧玺治理环境的用途,例如吸附污水中重金属离子、降解有极大分子污染物等.人体佩戴碧玺时,这种自发极化现象也会带来一定的保健功效,具有一定的电磁屏蔽效果,促进人体新陈代谢.  相似文献   

光纤光栅应变传感器在地质灾害上的应用     

曾克 《物探与化探》2014,(1):142-144,156

根据光纤光栅传感的原理,提出了光纤光栅式封装应变传感器,对其传感特性进行了研究,并进行了室内实验。结合光栅传感监测滑坡的应用实例,探讨了光纤布拉格光栅传感元件在滑坡体上的布设工艺及监测过程。分析初期的监测结果,针对监测系统可能出现的问题提出了解决途径。  相似文献   

新场须四段叠后裂缝综合预测     

王丹  贾跃玮  魏水建  郑文波 《物探与化探》2014,(5):1038-1044

叠前裂缝预测方法主要针对垂缝和高角度缝,而川西新场须四下亚段致密砂岩储层裂缝以低角度缝为主,叠前方法在本工区不再适用;而单一叠后属性的裂缝预测方法可靠性差,因此,笔者提出了一套叠后裂缝综合预测新方法:首先基于多属性聚类分析进行裂缝地震相分级,并利用实测资料进行监控,从而实现多属性、多尺度裂缝综合定性预测;然后对滤掉基质相的曲率数据计算蚂蚁体,减小基质相对蚂蚁追踪的影响,从而得到能识别小尺度裂缝且裂缝形态更加清晰的高精度蚂蚁体;最后,基于高精度蚂蚁体建立三维裂缝模型,对裂缝发育特征进行半定量预测。实际应用结果表明:基于叠后资料的新一套裂缝综合预测思路在新场地区应用效果好,有效解决了低角度缝难预测的问题。  相似文献   

大尹格庄金矿床矿体三维建模与矿化分布规律          下载免费PDF全文

陈东锋  邹艳红  毛先成  陈进  吴泽权 《地质找矿论丛》2014,29(4):527-534

文章根据勘探线地质剖面图钻孔样品化验数据和中段地质平面图坑道样品化验数据,利用Vulcan软件对大尹格庄金矿床矿体建立了两种三维实体模型,并将这两种模型结合起来,利用Datamine软件得到综合后的块体模型;运用地质统计学方法及Surpac软件,分析了①、②号两个矿（脉）体群的Au品位空间变化结构,并求得了搜索椭球体,实现了矿体和Au品位变化形态的空间分布展示;结合三维建模成果与矿体空间变化结构,分析得出了矿化分布规律.②号矿（脉）体群沿NE向继续展布的区域,是寻找深部隐伏矿体的有利部位.  相似文献