利用LaBr3（Ce）伽马谱仪直接测定铀矿体中铀含量的方法     

吴永鹏  汤彬  程建平  梁永顺  王哲 《物探与化探》2012,36(3):414-417

LaBr3（Ce）闪烁体是一种综合性能优良的新型伽马射线探测器。然而,以它的能量分辨性能还不能获得含铀矿体精细伽马谱,其仪器谱反映不出与铀含量直接相关的特征峰,在这种情况下,探索一种直接获取含铀矿体铀含量的方法。采用国产LaBr3（Ce）探头对系列硬岩型放射性矿体进行测量,通过234Pam之1.001 MeV伽马特征能量以能量窗结合线性回归的相对分析法直接求取铀等目标核素的含量,获得了良好效果,对硬岩型铀矿含铀99×10^-6以上相对误差不超过10.0%,对矿体中其他主要核素的定量分析误差也在8.5%以内。  相似文献   

大功率多道密集排列滚动方式三极测深在地灾隐患勘查中的应用          下载免费PDF全文

朱向泰  刘亚军  韩艳军 《地质找矿论丛》2012,27(2):251-259

大功率多道密集排列滚动方式三极测深是在传统电测深法基础上经过装置变换、改进而来的新型实用测深技术,相比常规的高密度直流电法,具有探测深度大、横向分辨率高、提供信息丰富(可同时提供视电阻率、充电率)、抗干扰能力强等特点,近几年广泛应用于多金属矿勘查、地质隐患调查、工程地质探查等领域,文章介绍了该方法的装置特点和工作流程,...  相似文献   

板状体MT倾子响应的二维有限元模拟与定性分析     

柳建新  甘佳雄  童孝忠  曹创华  籍炜 《物探化探计算技术》2012,34(5):541-547

在二维地电模型中,大地电磁测深倾子资料可以很好地反映地电构造的水平非均匀性,特别是在解释垂直或者倾斜板状体的空间分布情况时,可以起到十分重要的作用,在实际应用中可以用来寻找断裂,判断其走向、倾向、埋深和规模。应用有限单元法分别对水平、垂直和倾斜的板状模型进行正演模拟,该算法采用矩形网格内进一步三角形细化的方式剖分模型,通过三角形网格提高了对倾斜接触面的近似程度,同时增加计算量不明显,然后计算出倾子的实部、虚部和振幅的资料。研究结果表明:倾子响应对介质电性水平不均匀反映十分灵敏,特别是对横向低阻异常体,同时对异常体的位置和埋深也有清楚的显示。  相似文献   

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