Microscopy and rock magnetism of fine grain-size titanomagnetite from the Jacupiranga Alkaline Complex,Brazil: unearthing Ti-magnesioferrite nanoparticles     

Luis M. Alva-Valdivia  María de la Luz Rivas-Sánchez  Jesús Arenas-Alatorre  Avto Goguitchaishvili  Omar Ferreira Lopes 《Geofísica Internacional》2013,52(2):93-110

Very fine samples from the mineralized zones of the Jacupiranga complex at the Cajati mine were selected for crystallographic identification of Ti-magnesioferrite (TMf) nanostructures embedded in titanomagnetite (TM) using high-resolution transmission electron microscopy (TEM). A magnetic concentrate obtained of pyroxenite samples (sites 4 to 7) was reduced and divided into fractions of distinct range sizes: 26±2 μm, 19±1 μm, 13±1 μm, 9±1 μm, 6±1 μm and 6-0.1 μm. The mineralized samples of carbonatite and pyroxenite were characterized by X-ray diffraction, transmitted and reflected light microscope, and scanning electron microscope with multielemental analysis. The finest magnetic concentrate sample (MC₆) was analyzed under high-resolution transmitted electron microscopy (TEM) and high angle annular dark field and Raman spectroscopy. Magnetic properties were measured for the distinct granulometric fractions, showing drastic changes when grain sizes go beyond the frontier from micro to nanometer sizes. Frequency-dependent magnetic susceptibility percentage (÷_fd%) report higher values (10.2%) for the finer fractions (6±1 μm and 6-0.1 μm) attributed to dominant fractions of superparamagnetic particles. Nanometer and < 6 μm grain size TMf in TM particles require a magnetic field up to 249 mT to reach saturation during the isothermal remanent magnetization experiment. Coercivity and remanent magnetization of these samples increase when the particle size decreases, probably due to parallel coupling effects. Magnetic susceptibility versus temperature experiments were conducted two times on the same (< 35 nm) sample, showing that the repetition during the second heating is probably due to the formation of new TMf nanoparticles and growth of those already present during the first heating process.  相似文献   

早子沟金矿矿石质量特征、选矿试验研究及选别效果   总被引：1，自引：0，他引：1  

刘春先  陈耀宇  柳生祥  梁志录  金鼎国 《甘肃地质》2012,(2):57-62

本文依据早子沟金矿矿区勘查及选矿工艺矿物学研究资料,从金矿石的结构构造、矿石类型、矿物成分、金的赋存状态及其主要载体矿物的嵌布特征、共伴生组分等方面综述了矿石质量特征,重点分析了以上矿石质量特征要素对选矿的影响;简述了选矿试验研究的成果及选别效果。矿区矿石工艺类型属少硫化物微细粒浸染型含金矿石,金的赋存状态复杂,利用重选—浮选中矿再磨的重浮联合流程可获得较理想的选冶回收指标。  相似文献   

阿尔泰南缘中泥盆统北塔山组火山岩的矿物学研究   总被引：2，自引：0，他引：2  

张贺  张招崇 《矿物学报》2012,32(3):386-397

阿尔泰山南缘中泥盆统北塔山组火山岩极为发育。本文对富辉橄玄岩和玄武岩中的单斜辉石和橄榄石斑晶进行了矿物化学分析,并结合矿物的地质温压计和岩浆结晶模拟,约束了两种岩石中矿物的形成过程,推测了原始岩浆的演化过程。提出富辉橄玄岩和玄武岩的原始岩浆属于拉斑玄武系列,富辉橄玄岩中的高压单斜辉石来源于深部（40～50 km）,其结晶早于橄榄石;玄武岩中单斜辉石大多属于岩浆房结晶产物（30～40km）,其结晶晚于橄榄石;两种岩石中橄榄石均属于岩浆房结晶产物（30～40 km）。  相似文献   

贵州威宁沉积型赤铁矿矿石工艺矿物学研究     

刘贞才  谯文浪  安亚运  陈武  王波 《贵州地质》2012,29(1):62-67

对贵州威宁沉积型赤铁矿石进行了工艺矿物学研究,重点研究了该矿石的矿物组成、主要矿物嵌布特征和主要含铁矿物赤铁矿的单体解离情况。研究表明,该矿石属于低磷、低硫、微细粒嵌布的赤铁矿石;矿石中主要铁矿物以赤铁矿为主,其次为磁铁矿和褐铁矿,主要脉石矿物以石英为主,其次为绿泥石、云母、高岭石等粘土矿物;赤铁矿嵌布粒度极细,平均粒度0.015mm,且赤铁矿与脉石矿物嵌布关系复杂。本研究为该矿石的开发利用提供基础资料。  相似文献   

SCI收录的矿物学类核心期刊介绍     

王彦 《矿物学报》2012,32(2):316-320

以表格的形式汇总介绍了SCI收录的20种矿物学类目核心期刊的刊名、国际标准刊号（ISSN）、出版地和最新影响因子,并详细介绍了这20种期刊的出版周期、出版者、联系地址、最新期刊网址及期刊描述等全方位的期刊信息。期刊描述内容包括：期刊的创刊年以及期刊的发展,期刊刊载的主要内容,网站可免费获取的该刊目次和文摘及全文信息等,以便为相应学科的科研工作者提供参考。  相似文献   

西藏尼雄矿田日阿铜矿床矽卡岩矿物学特征及地质意义   总被引：3，自引：1，他引：2  

于玉帅  杨竹森  刘英超  田世洪  赵灿  高原  纪现华  胡为正  曹圣华 《矿床地质》2012,31(4):775-790

尼雄矿田位于冈底斯成矿带西段中部隆格尔南木林岩浆岩带的北侧.日阿铜矿床位于尼雄矿田的东南端,矿体产于晚白垩世侵入岩与下拉组灰岩接触带的矽卡岩或矽卡岩化大理岩中,主要矽卡岩矿物有石榴子石、透辉石、蛇纹石、金云母、绢云母、硅镁石、阳起石、透闪石、绿帘石、绿泥石等.电子探针分析表明,矿区石榴子石主要为钙铁榴石,次为钙铝榴石;辉石以透辉石为主;金云母明显富镁贫铁,且富含挥发分F;闪石类矿物属钙角闪石系列;绿泥石富镁贫铁.推断成矿流体大致经历了5个演化阶段:①干矽卡岩阶段,高温(＞450℃)、低pH值、氧化-弱氧化;②湿矽卡岩阶段,温度降低,pH值和氧逸度逐渐升高;③氧化物阶段,温度进一步降低,pH值升高(碱性),氧逸度则呈降低趋势;④石英硫化物阶段,中等温度(200～300℃),高pH值(碱性),低氧逸度;⑤碳酸盐阶段,低温(160～203℃),低pH值,低氧逸度.此外,矿区还存在多金属矿化的可能.  相似文献   

Mineralogy and Mineral Chemistry of the Cretaceous Duolong Gold‐Rich Porphyry Copper Deposit in the Bangongco Arc,Northern Tibet     

Jinxiang LI  Guangming LI  Kezhang QIN  Bo XIAO  Lei CHEN  Junxing ZHAO 《Resource Geology》2012,62(1):19-41

The Early Cretaceous Duolong gold‐rich porphyry copper deposit is a newly discovered deposit with proven 5.38 Mt Cu resources of 0.72% Cu and 41 t gold of 0.23 g t^?1 in northern Tibet. Granodiorite porphyry and quartz diorite porphyrite are the main ore‐bearing porphyries. A wide range of hydrothermal alteration associated with these porphyries is divided into potassic, argillic and propylitic zones from the ore‐bearing porphyry center outward and upward. In the hydrothermal alteration zones, secondary albite (91.5–99.7% Ab) occurs along the rim of plagioclase phenocryst and fissures. Secondary K‐feldspar (75.1–96.9% Or) replaces plagioclase phenocryst and matrix or occurs in veinlets. Biotite occurs mainly as matrix and veinlet in addition to phenocryst in the potassic zone. The biotite are Mg‐rich and formed under a highly oxidized condition at temperatures ranging from 400°C to 430°C. All the biotites are absent in F, and have high Cl content (0.19–0.26%), with log (X_Cl/X_OH) values of ?2.74 to ?2.88 and IV (Cl) values of ?3.48 to ?3.35, suggesting a significant role of chloride complexes (CuCl₂^‐ and AuCl₂^‐) in transporting and precipitating copper and gold. Chlorites are present in all alteration zones and correspond mainly to pycnochlorite. They have similar Fe/(Fe+Mg), Mn/(Mn+Mg) ratios, and a formation temperature range of 280–360°C. However, the formation temperature of chlorite in the quartz‐gypsum‐carbonate‐chlorite vein is between 190°C and 220°C, indicating that it may have resulted from a later stage of hydrothermal activity. Fe³⁺/Fe²⁺ ratios of chlorites have negative correlation with Al^IV, suggesting oxygen fugacity of fluids increases with decreasing temperature. Apatite mineral inclusions in the biotite phenocrysts show high SO₃ content (0.44–0.82%) and high Cl content (1–1.37%), indicating the host magma had a high oxidation state and was enriched in S and Cl. The highest Cl content of apatite in the propylitic zone may have resulted from pressure decrease, and the lowest Cl content of apatite in the argillic zone may have been caused by a low Cl content in the fluids. The low concentration of SO₃ content in the hydrothermal apatite compared to the magmatic one may have resulted from the decrease of oxygen fugacity and S content in the hydrothermal fluid, which are caused by the abundant precipitation of magnetite.  相似文献   

ERP精度对“嫦娥一号”差分VLBI定位精度的影响   总被引：2，自引：0，他引：2  

魏二虎  史青  严韦  李雪川 《武汉大学学报(信息科学版)》2011,36(11):1324-1327,1387

推导了差分VLBI（ΔDOR）用于月球探测器定位的数学模型,利用嫦娥一号实测数据对探测器的位置和地球自转参数（ERP）同时进行了解算,并分析了ERP先验精度对定位精度的影响。  相似文献   

The Rumuruti chondrite group     

Addi Bischoff  Nadia Vogel  Julia Roszjar 《Chemie der Erde / Geochemistry》2011,(2):101-133

Since 1994, the Rumuruti (R) chondrites have been recognized as a new, well-established chondrite group differing from carbonaceous, ordinary, and enstatite chondrites. The first R chondrite, Carlisle Lakes, was found in Australia in 1977. Meanwhile, the number has increased to 107 (December, 2010). This group is named after the Rumuruti meteorite, the first and so far the only R chondrite fall. Most of the R chondrites are breccias containing a variety of different clasts embedded in a clastic matrix. Some textural and mineralogical characteristics can be summarized as follows: (a) the chondrule abundance in large fragments and in unbrecciated rocks is ∼35–50 vol%; (b) Ca,Al-rich inclusions are rare; (c) the olivine abundance is typically 65–78 vol%; (d) the mean chondrule diameter is ∼400 μm; (e) in unequilibrated R chondrites, low-Ca pyroxene is dominating, whereas in equilibrated R chondrites it is Ca-rich pyroxene; (f) the typical olivine in a metamorphosed lithology is ∼Fa_38–40; (g) matrix olivine in unequilibrated, type 3 fragments and rocks has much higher Fa (∼45–60 mol%) compared to matrix olivines in type 4–6 lithologies (∼Fa_38–41); (h) spinels have a high TiO₂ of ∼5 wt%; (i) abundant different noble metal-bearing phases (metals, sulfides, tellurides, arsenides) occur. The exception is the metamorphosed, type 5/6 R chondrite La Paz Icefield 04840 which contains hornblende, phlogopite, and Ca-poor pyroxene, the latter phase typically occurring in low-grade metamorphosed R chondrites only.In bulk composition, R chondrites have some affinity to ordinary chondrites: (a) the absence of significant depletions in Mn and Na in R chondrites and ordinary chondrites is an important feature to distinguish these groups from carbonaceous chondrites; (b) total Fe (∼24 wt%) of R chondrites is between those of H and L chondrites (27.1 and 21.6 wt%, respectively); (c) the average CI/Mg-normalized lithophile element abundances are ∼0.95 × CI, which is lower than those for carbonaceous chondrites (≥1.0 × CI) and slightly higher than those for ordinary chondrites (∼0.9 × CI); (d) trace element concentrations such as Zn (∼150 ppm) and Se (∼15 ppm) are much higher than in ordinary chondrites; (e) the whole rock Δ¹⁷O of ∼2.7 for R chondrites is the highest among all meteorite groups, and the mean oxygen isotope composition is δ¹⁷O = 5.36 ± 0.43, δ¹⁸O = 5.07 ± 0.86, Δ¹⁷O = +2.72 ± 0.31; (f) noble gas cosmic ray exposure ages of R chondrites range between ∼0.1 and ∼70 Ma. More than half of the R chondrites analyzed for noble gases contain implanted solar wind and, thus, are regolith breccias. The 43 R chondrites from Northern Africa analyzed so far for noble gases seem to represent at least 16 falls. Although the data base is still scarce, the data hint at a major collision event on the R chondrite parent body between 15 and 25 Ma ago.  相似文献   

大地震的18.6年周期   总被引：1，自引：0，他引：1       下载免费PDF全文

杜品仁  赵俊猛  高祥林 《地球物理学报》2011,54(9):2256-2262

将全球分为15个研究区,用1900~2009年M_W≥7.0地震目录,统计分析了各区大地震与月球交点运动周期的关系,得出15个研究区中有10个区,大地震存在统计意义上的18.6 a周期:活跃段为12.4 a,平静段为6.2 a;环太平洋地震带北、南、西、东4大区的大地震,不仅有这样的周期,而且其地震活跃段的时间存在一定规律.用第6个18.6 a(1991~2009年)期间的大地震,检验据前5个18.6 a(1900~1990年)地震目录所得18.6 a 周期的稳定性和实用性,发现有这种周期的地区多数的周期性是稳定的.大地震18.6 a周期的可能成因有: (1)18.6 a潮波通过调制日潮和半日潮调制大地震; (2)上地幔内流体的潮汐(地内潮)作用; (3)18.6 a潮波通过影响地球自转变化调制大地震.  相似文献