重要找矿指示元素的野外快速分析法——金的野外快速分析     

卢荫庥  王晓苓 《物探与化探》1993,17(6):449-455

近年来,作者发展了七种以上重要找矿指示元素的野外快速分析法,此乃其一。文中提出一种新的金样冷浸技术,引进了新的光导光度检测方法,样品经溴化钠—硫酸—过氧化氢冷浸,用经丙酮—MIBK处理的泡沫塑料富集金,经混合解脱剂解脱并直接取解脱液用改进的微珠析出法或用光导光度法测定。取10g样品,可测定0.0005-50g/t范围内的金。方法简便、快速,可在普查分队驻地进行,每一工作日可测定80多个样品,由于废弃了王水分解样品和泡沫塑料的灰化,具有广阔的应用前景。  相似文献   

地震前兆含义,科学问题与研究途径的研讨   总被引：5，自引：2，他引：3  

张肇诚  王贵宣 《地震》1997,17(4):429-439

地震前兆的研究已经取得了很大的进展,地震前兆的复杂性引起了广泛的关注,对地震预报、有关科学问题和探索途径的研究现状及其前景有各种评价。文章认为由于一些科学问题没有解决,尽管对中缅边境１９９５年７月连７．３级地震作出了成功预报,经验性预报有一定的局限性,文中讨论了广义地震前兆和狭义地震前兆,广义地震前兆包含二类前兆：场兆和源兆;而狭义前兆仅指后者。大陆震例前兆的系统研究证实了广义地震前兆的存在,然而  相似文献   

TheROSAT survey of extreme UV sources: a new window on the universe     

David A. H. Buckley 《Astrophysics and Space Science》1995,228(1-2):349-365

This paper discusses the first all-sky suvey of cosmic extreme ultra-violet sources, discovered by theROSAT Wide Field Camera. Details of the instrument and the survey are presented, with comparisons made to previous selected surveys in the X-ray regime. The subsequent optical identification program is described, and the major results summarized. I then discuss the main classes of EUV emitters: active chromosphere stars and hot white dwarfs, and describe the importance of EUV obserevations in understanding the astrophysics of these objects. Many bright, and relatively nearby, sources have been identified with hitherto unrecognized active stars, representing the extremes in chromospheric and coronal activity, be it binary or age related. Many new hot DA white dwarfs have also been indentified, and the most exciting result in this area is the discovery that significant traces of heavier elements (e.g. C, N, O, Si, Fe & Al) exist in their atmospheres, substantially increasing their EUV opacities. The importance of hot white dwarfs as standard candles in probing the local interstellar medium is also discussed. Miscellaneous counterparts (AGN, PNN, O-B stars and CVs) that make up the rest of the sample of EUV sources are also briefly mentioned. I conclude the paper with a discussion of the new magnetic cataclysmic variables discovered at SAAO, which have been the subject of intensive follow-up observations.  相似文献   

The circumstellar shells of carbon miras     

Martin Groenewegen 《Astrophysics and Space Science》1995,224(1-2):321-324

The relation between mass loss rate and pulsation period in carbon Miras is discussed. The dust mass loss rate is very low (about 2 × 10^–10 M/yr) up to aboutP = 380 days, where there is a sudden increase. ForP > 400 days there is a linear relation between logM andP. The change in the mass loss rate near 380 days may be related to radiation pressure on dust becoming effective in driving the outflow.  相似文献   

Lermontovskoe Tungsten Skarn Deposit: the Oldest Mineralization in the Sikhote-Alin Orogen, Far East Russia     

Kohei Sato    Sergei M. Rodionov  Anatoly A. Brublevsky 《Resource Geology》2006,56(3):257-266

Abstract. Lermontovskoe tungsten skarn deposit in central Sikhote-Alin is concluded to have formed at 132 Ma in the Early Cretaceous, based on K-Ar age data for muscovite concentrates from high-grade scheelite ore and greisenized granite. Late Paleozoic limestone in Jurassic - early Early Cretaceous accretionary complexes was replaced during hydrothermal activity related to the Lermontovskoe granodiorite stock of reduced type. The ores, characterized by Mo-poor scheelite and Fe^3+- poor mineral assemblages, indicate that this deposit is a reduced-type tungsten skarn (Sato, 1980, 1982), in accordance with the reduced nature of the granodiorite stock.
The Lermontovskoe deposit, the oldest mineralization so far known in the Sikhote-Alin orogen, formed in the initial stage of Early Cretaceous felsic magmatism. The magmatism began shortly after the accretionary tectonics ceased, suggesting an abrupt change of subduction system. Style of the Early Cretaceous magmatism and mineralization is significantly different between central Sikhote-Alin and Northeast Japan; reduced-type and oxidized-type, respectively. The different styles may reflect different tectonic environments; compressional and extensional, respectively. These two areas, which were closer together before the opening of the Japan Sea in the Miocene, may have been juxtaposed under a transpressional tectonic regime after the magmatism.  相似文献   

A review of the adjoint-state method for computing the gradient of a functional with geophysical applications   总被引：8，自引：0，他引：8  

R.-E. Plessix 《Geophysical Journal International》2006,167(2):495-503

  相似文献   

环境样品中痕量元素的化学形态分析Ⅰ．分析技术在化学形态分析中的应用   总被引：21，自引：7，他引：21  

何红蓼 李冰杨红霞  倪哲明 《岩矿测试》2005,24(1):51-58

文章介绍了形态分析的基本概念,常用的联用分析技术,如气相色谱原子吸收光谱、气相色谱原子荧光光谱、气相色谱微波诱导等离子体原子发射光谱、气相色谱电感耦合等离子体质谱、高效液相色谱电感耦合等离子体质谱等在环境样品(水、土壤、沉积物)中痕量元素化学形态(价态、金属有机化合物等)分析中的应用,土壤和沉积物中污染元素的顺序提取步骤,以形态分析发展动态。引用文献72篇。  相似文献   

新疆绿色电气石颜色成因研究   总被引：5，自引：0，他引：5       下载免费PDF全文

王进军陶晓风  王武军 《岩石矿物学杂志》2005,24(4):319-323

新疆绿色电气石颜色成因比较特殊,为了更好地了解其颜色的形成,主要采用化学分析、吸收光谱、穆斯堡尔谱等测试手段对绿色电气石颜色成因进行研究。化学分析结果显示每个样品中均含有少量不同过渡元素离子,如Fe2 、Ti4 、Cr3 等,影响着绿色的形成;利用吸收光谱测试方法确定了致色离子的吸收带位置及主要离子的种类、价态,并根据化学成分计算出相应的化学式,利用穆斯堡尔谱确定了铁离子在晶体中的占位。综合运用上述测试方法,确定了绿色电气石的颜色成因。  相似文献   

中国大陆科学钻探主孔声发射法现今地应力状态的确定   总被引：9，自引：0，他引：9       下载免费PDF全文

王连捷李朋武  崔军文丁原辰 《中国地质》2005,32(2):259-264

对中国大陆科学钻探主孔的岩心进行了声发射测量,确定了301～1531m深度的最大主应力。并与钻孔崩落法(深度1269～1655m)测量结果进行了对比,结果表明,声发射测量所得测值基本上落在钻孔崩落法测值的趋势线上,两种方法所得结果一致,说明测量结果可信。测量结果表明科学钻探主孔地应力大小随深度增加,在浅部301m最大主应力为13.4MPa,在深部1655m为55.2MPa。随深度的增加率为0.0279MPa/m。最大主应力方向为N54°±3.3°E,且方向不随深度变化。  相似文献   

大气热力学的若干新发展          下载免费PDF全文

曹鸿兴 《应用气象学报》2005,16(4):554-416

对自20世纪80年代以来的大气热力学发展进行了综合评述, 阐述了如城市热岛效应、全球增暖等非传统大气热力学问题; 基于大气非平衡态热力学的非线性理论, 提出应发展突显热力学作用的数值模式, 并阐述其必要性和可能性。  相似文献