四川昭觉县中部乡镇表层土壤硒地球化学特征     

赵辰  孙彬彬  贺灵  吴超  成晓梦  曾道明  刘冬 《岩矿测试》2022,(3):412-426

硒元素是人体必需的微量元素之一,食用富硒农产品是人体获取和补充硒元素的主要途径,调查区域硒地球化学特征是有效地利用富硒土地资源以及开发富硒农副产品的重要依据。本文选择四川省昭觉县域内较为重要的农耕乡镇采集表层土壤样品,采用原子荧光光谱法、X射线荧光光谱法、电感耦合等离子体质谱/发射光谱法等方法测定1328件土壤、19件玉米及20件土豆中硒等地球化学指标含量,利用相关分析与统计学等方法,结合距离加权反比插值法,探讨研究区硒含量、分布和影响因素等地球化学特征,评价土壤与作物的富硒情况及安全性。结果表明：(1)研究区表层土壤硒含量范围为0.04～1.50mg/kg,平均值为0.33mg/kg,划定富硒土壤面积为7.23km~2,占全区土壤面积的30.31%,玄武岩发育的土壤硒含量最高,平均值为0.4mg/kg,表明区内地质背景与土壤硒含量密切相关,区内富硒土壤主要受含玄武岩夹苦橄岩、凝灰质砂泥岩的峨眉山玄武岩组地层控制;(2)不同的用地类型和土壤类型对硒元素的富集能力不同,人为农业活动导致土壤对硒的吸附能力下降,黄棕壤土层中黏粒或铁氧化物等易与硒结合富集;酸性土壤中硒含量与pH值成反比;土壤...  相似文献   

利用X射线粉晶衍射和电感耦合等离子体质谱法研究江西西华山钨矿床中黑钨矿的矿物学特征及指示意义     

鲁麟  梁婷  陈郑辉  王勇  黑欢  谢星 《岩矿测试》2015,34(1):150-160

目前针对江西大型黑钨矿石英脉型钨矿床西华山的黑钨矿矿物学特征及指示意义研究较少。本文利用X射线粉晶衍射分析和电感耦合等离子体质谱分析技术对黑钨矿晶体结构、化学成分特征及空间变化规律开展研究。获得黑钨矿晶胞参数为a0=0.477 nm,b0=0.573 nm,c0=0.498 nm,β=90°21',属于锰钨铁矿,与前人得出的黑钨矿晶胞参数略有不同,代表不同元素对铁锰的类质同象替代。主要化学成分WO3、Fe O、Mn O的含量在空间上具有一定的变化规律,反映了成矿物质的运移特征。微量元素Sc、Y、Nb、Ta在垂向含量变化大,说明矿液运移具有复杂性。稀土总量ΣREEs较高(397.16×10-6~1071.11×10-6),具有强烈的Eu负异常,具重稀土富集左倾的"躺椅式"球粒陨石标准化配分模式。将西华山、盘古山、淘锡坑、大吉山4个典型矿床的黑钨矿稀土元素特征进行对比,反映产在花岗岩内接触带的黑钨矿的稀土总量(ΣREEs)相对最高,分馏最明显;产在花岗岩内及其外接触带的黑钨矿的稀土总量(ΣREEs)相对较低,分馏程度最不明显;而产在花岗岩外接触带的黑钨矿的稀土总量(ΣREEs)有高有低,分馏程度有强有弱。因此,黑钨矿的化学成分变化特征,可以有效地指示成矿物质空间运移特征、物质来源和矿床成因。  相似文献   

红土镍矿样品前处理方法和分析测定技术研究进展     

燕娜  赵小龙  赵生国  郑红文 《岩矿测试》2015,34(1):1-11

随着常规镍来源的硫化镍矿资源的日益枯竭,可直接生产氧化镍、镍锍和镍铁等产品的红土镍矿倍受关注。对于红土镍矿中主量、次量、痕量元素的检测,相同的检测项目存在多种测试方法,且部分相同原理的测试方法存在细节上的差异,使得检测者选择合适的检测方法变得困难。本文综述了近年来红土镍矿中24种元素测定的样品前处理方式及分析技术研究进展。样品前处理方式依据目标元素及后续的分析方法进行选择,其中酸溶法和碱熔法用途最广。酸溶法引入的盐分少,操作简单,但是分解过程中易导致挥发元素As、Sb、Bi、Hg的损失,Cr易随高氯酸冒烟损失。碱熔法分解能力强,适合分析Cr、Si、全铁等项目,但会引入大量的盐类和因坩埚材料损耗而带入其他杂质,给后续分析带来困难。红土镍矿的分析技术依据实验室条件及目标元素的性质和浓度进行选择。电感耦合等离子体发射光谱法(ICP-AES)是主量、次量元素的主要分析方法,适合于分析含量为10-5~30%级别的金属元素;X射线荧光光谱法主要用于分析含量为10-3~1级别的元素,尤其适合于测定Al、Si、Ti、V和P,由于该方法的准确性依赖于一套高质量的标准样品,故更适合炉前检测或检测大批红土镍矿样品。电感耦合等离子体质谱法(ICP-MS)最适合于分析10-4含量以下的重元素,特别是稀土和贵金属元素。原子吸收光谱法(AAS)适合于分析10-4~10-2级别的Ca、Mg、Ni、Co、Zn、Cr、Mn等低沸点、易原子化元素。分光光度法主要用于分析Ni和P。原子荧光光谱法(AFS)主要用于分析As、Bi、Sb等易形成气态氢化物的元素。容量法主要用于分析Al、Fe、Mg和Si O2等主含量元素。尽管AAS、分光光度法、AFS法和容量法检测周期长,但所用仪器为实验室常规配置,可满足缺乏相应大型仪器实验室的日常检测。本文认为,针对各种检测方法的适用性及存在问题,应从开发微波消解法、固体进样直接测汞法、ICP-MS法以及Cr与其他元素同时分析的快速分析方法等方面开展研究,建立灵敏、准确的检测方法,从而更好地服务于红土镍矿的贸易、检验和综合利用。  相似文献   

应用FTIR-XRD-XRF分析测试技术研究新型仿制绿松石的矿物学特征   总被引：4，自引：3，他引：1  

严俊  刘晓波  王巨安  方飚  刘培钧  杨彬彬 《岩矿测试》2015,34(5):544-549

近年来绿松石及其仿制品的鉴定工作较多局限于应用傅里叶变换红外光谱对仿制品进行简单的筛选,前人报道的仿制绿松石的矿物组成主要为单一的矿物相(如异极矿、三水铝石、磷铝石、羟硅硼钙石、菱镁矿等)。本文应用傅里叶变换红外光谱(FTIR)、X射线粉晶衍射(XRD)与X射线荧光光谱(XRF)对当前珠宝市场上几种新型仿制绿松石进行了初步分类,并对不同类别的仿制绿松石的具体矿物组成、物相及晶型特征作了对比研究。结果表明,这些新型仿制绿松石可分为三大类:一类主要由硅酸盐(斜硅钙石)与碳酸盐(方解石)两种矿物组成;另一类为白云石与方解石两种碳酸盐矿物的混合相;第三类以硅酸盐类为主要矿物,并含有钡长石、辉石与石英。显然,新型仿制绿松石的矿物组成明显相异于传统仿制品,可见仿制绿松石的矿物组成日趋多样性、复杂化,该现状必然对新型仿制样品的物相鉴定提出了更高的要求。  相似文献   

利用X射线衍射和岩矿鉴定等技术研究河南汤家坪钼矿区主要矿物标型特征   总被引：1，自引：1，他引：0  

周姣花  汪建宇  顾茗心  王真 《岩矿测试》2015,34(1):82-90

汤家坪钼矿床是2006年探明的一处大型斑岩型钼矿床,前人用常规地质方法对该矿区基础地质工作和成矿规律研究已比较系统和完整,认为汤家坪钼矿床属于深源浅成斑岩型钼矿床,汤家坪花岗斑岩体为矿区钼矿的成矿母岩;但是没有从矿物学角度来应证这些成矿规律。本文从矿物学角度,采用分离单矿物进行化学分析、X射线衍射(XRD)及岩矿鉴定等技术,对汤家坪钼矿区的辉钼矿、黄铁矿、石英、长石4种矿物标型特征(化学组成、微量元素、晶体结构、晶胞参数、结构状态等)进行研究。结果表明:1该矿区辉钼矿全部是2H型多型变体,且成分中Re含量很低;辉钼矿的δ34S值为3.0‰,硫同位素变化范围小,接近于陨石硫,具深源硫的特点,硫来源于花岗斑岩。2黄铁矿微量元素以富含Mo、Co、Cu,贫Ni、Pb、Zn为标型特征,另外Au、Ag含量低,S/Se大于250000,与前人"S/Se大于250000~500000的地区不可能找到金矿"的结论相符。3石英富含Mo;成矿期石英脉中δ18O降低,表明成矿晚期有少量大气降水参与热液蚀变成矿。4长石富含Mo;轻稀土(La~Nd)含量大于中稀土(Sm~Ho)和重稀土(Er~Y)含量;钾长石的有序度、三斜度以及结构参数的值均较高,结构温度较低,表明该矿区钾长石为低温状态下的三斜对称的微斜长石,是热液作用的产物,岩体钾长石化对钼矿化最为有利。本研究应证了汤家坪钼矿床属于深源浅成斑岩型钼矿床,对于总结斑岩型钼矿成矿规律、找矿标志有重要意义。  相似文献   

Distribution and partitioning of major and trace elements in pyrite-bearing sediments of a Mediterranean coastal lagoon     

《Chemie der Erde / Geochemistry》2015,75(2):219-236

The formation of iron sulphide minerals exerts significant control on the behaviour of trace elements in sediments. In this study, three short sediment cores, retrieved from the remote Antinioti lagoon (N. Kerkyra Island, NW Greece), are investigated concerning the solid phase composition, distribution, and partitioning of major (Al, Fe) and trace elements (Cd, Cu, Mn, Pb, and Zn). According to ²¹⁰Pb, the sediments sampled correspond to depositions of the last 120 years. The high amounts of organic carbon (4.1–27.5%) result in the formation of Fe sulphides, predominantly pyrite, already at the surface sediment layers. Pyrite morphologies include monocrystals, polyframboids, and complex FeS–FeS₂ aggregates. According to synchrotron-generated micro X-ray fluorescence and X-ray absorption near-edge structure spectra, authigenically formed, Mn-containing, Fe(III) oxyhydroxides (goethite type) co-exist with pyrite in the sediments studied. Microscopic techniques evidence the formation of galena, sphalerite and CuS, whereas sequential extractions show that carbonates are important hosts for Mn, Cd, and Zn. However, significant percentages of non-lattice held elements are bound to Fe/Mn oxyhydroxides that resist reductive dissolution (on average 60% of Pb, 46% of Cd, 43% of Zn and 9% of Cu). The partitioning pattern changes drastically in the deeper part of the core that is influenced by freshwater inputs. In these sediments, the post-depositional pyritization mechanism, illustrated by overgrowths of Fe monosulphides on pre-existing pyrite grains, results in relatively high degree of pyritization that reaches 49% for Cd, 66% for Cu, 32% for Zn and 7% for Pb.  相似文献   

A Fundamental Plane of Black Hole Activity: Pushing Forward the Unification Scheme     

Andrea Merloni  Sebastian Heinz  Tiziana Di Matteo 《Astrophysics and Space Science》2005,300(1-3):45-53

We examine the disc-jet connection in stellar mass and supermassive black holes by investigating the properties of their compact emission in the hard X-ray and radio bands. We compile a sample of ∼100 active galactic nuclei with measured mass, 5 GHz core emission, and 2–10 keV luminosity, together with eight galactic black holes with a total of ∼50 simultaneous observations in the radio and X-ray bands. Using this sample, we study the correlations between the radio (L_R) and the X-ray (L_X) luminosity and the black hole mass (M). We find that the radio luminosity is correlated with both M and L_X, at a highly significant level. We show how this result can be used to extend the standard unification by orientation scheme to encompass unification by mass and accretion rate.  相似文献   

A possible line-like emission feature at 8 keV in the Seyfert 1.2 UGC 3973     

L. C. Gallo  A. C. Fabian  Th. Boller  W. Pietsch 《Monthly notices of the Royal Astronomical Society》2005,363(1):64-70

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Dynamics and radiation of young type-Ia supernova remnants: Important physical processes     

Sorokina  E. I.  Blinnikov  S. I.  Kosenko  D. I.  Lundqvist  P. 《Astronomy Letters》2004,30(11):737-750

Astronomy Letters - We analyze the physical processes that should be taken into account when modeling young type-Ia supernova remnants (SNRs) with ages of several hundred years in which forward...  相似文献   

A COMBINED REFRACTION-DIFFRACTION-DISSIPATION MODEL OF WAVE PROPAGATION   总被引：7，自引：0，他引：7  

楼菁 《中国海洋湖沼学报》1994,12(4):361-371

A numerical model based on the mild-slope equation of water wave propagation over complicated bathymetry,taking into account the combined effects of refraction,diffraction and dissipation due to wavebreaking is presented.Wave breaking is simulated by modifying the wave height probability density func-tion and the wave energy dissipation mechanism is parameterized according to that of the hydraulic jumpformulation.Solutions of the wave height,phase function,and the wave direction at every grid point areobtained by finite difference approximation of the governing equations,using Gauss-Seidel Iterative Method(GSIM)row by row.Its computational convenience allows it to be applied to large coast regions tostudy the wave transformation problem.Several case studies have been made and the results compare verywell with the experiment data and other model solutions.The capability and utility of the model forreal coast areas are illustrated by application to a shallow bay of northeast Australia.  相似文献