3,5—二溴—4—偶氮变色酸苯荧光酮与铝显色反应及应用

研究了在阳离子表面活性剂ＣＴＭＡＢ存在下，Ａｌ与３，５－二溴－４－偶氮变色酸苯基荧光酮的是色反应条件和光变性质。在ｐＨ６．０的ＨＡｃ－ＮａＡｃ缓冲介质中，Ａｌ与试剂形成１：２的红色配合物，最大吸收峰位于５６０ｎｍ处，表观摩尔吸光系数为１．２５×１０＾４Ｌ．ｍｏｌ＾－１．ｃｍ＾－１，Ａｌ的质量浓度为０－０．２ｍｇ／Ｌ时符合比尔定律。     

镁—4,5—二溴苯基荧光酮络合吸附波及其应用

在ＰＨ１０．３的ＮａＢ４Ｏ７－ＮａＯＨ介质中,Ｍｇ＾２＋与４,５－二溴苯基荧光酮形成络合物,于－０．９５Ｖ出现一灵敏的阴极波。Ｍｇ＾２＋的质量浓度在８．２－５８μｇ／Ｌ时与峰电流呈线性关系,检出限为２．１μｇ／Ｌ。     

二安替比林基—（3—溴）苯基甲烷与铈（Ⅳ）显色反应的研究

合成了二安替比林基－（３－溴）苯基甲烷。在Ｍｎ和吐温－８０存在下，Ｃｅ与ＤＡｍＢＭ反应生成有色化合物，λｍａｘ为３８０ε为３．０×１０＾５Ｌ．ｍｏｌ＾－１，ｃｍ＾－１。Ｃｅ量在（０－１０）μｇ／２５ｍｌ间符合比尔定律。     

5‘—硝基水杨基荧光酮与锆显色反应及其应用

在０．０８￣０．１０ｍｏｌ／Ｌ ＨＣｌ介质中，溴化十六烷基三甲铵（ＣＴＭＡＢ）存在下，Ｚｒ（Ⅳ）与５＇－硝基水杨基荧光酮（５＇－ＮＳＦ）发生显色反应，形成１：４的桔红色络合物，λｍａｘ＝５４０ｎｍ，ε为１．４６×１０＾５Ｌ·ｍｏｌ＾－１·ｃｍ＾－１，Ｚｒ（Ⅳ）含量在０￣０．５ｍｇ／Ｌ符合比尔定律。方法用于氧化铝及陶瓷釉料中锆的测定，结果与ＩＣＰ－ＡＥＳ法相符，ＲＳＤ（ｎ＝５）在１．３％￣３．７％。     

2,4—二溴—6—羧基苯重氮氨基偶氮苯光度法测定痕量铊的研究

研究了新试剂２，４－二溴－６－羧基苯重氮氨曲偶氮苯与Ｔｌ（Ⅲ）的高灵敏显色反应。在非离子表面活性剂ＴｒｉｔｏｎＸ－１００存在下，于ｐＨ１０．５的ＮＨ３．Ｈ２Ｏ－ＮＨ４Ｃｌ缓冲介质中，Ｔｌ（Ⅲ）与该试剂生成红色配合物，其配合物的最大吸收波长位于５２０ｎｍ处，摩尔吸光系数为１．８３×１０＾５Ｌ．ｍｏｌ＾－＾１．ｃｍ＾－＾１。Ｔｌ（Ⅲ）量在０－０．６４μｇ／ｍｌ范围内符合比尔定律。方法用于废水中痕量Ｔｌ     

钼—氨三乙酸—溴邻苯三酚红—溴化十六烷基三甲基铵体系的显色反应及其应用

在ＰＨ２．５的氯乙酸缓冲介质中，有溴化十六烷基三甲基胺存在下，Ｍｏ与氨三乙酸及溴邻苯三酚红形成胶束混配配合物，该配合物最大吸收波长在６００ｎｍ，摩尔吸光系数为７．２７×１０＾４Ｌ．ｍｏｌ＾－１．ｃｍ＾－１，配合物组成为Ｍｏ（Ⅵ）：ＮＴＡ：ＢＰＲ：ＣＴＭＡＢ＝１：１：２：４。Ｍｏ（Ⅵ）量在０－１．０μｇ／ｍｌ范围内符合比尔定律。由于ＮＴＡ的存在，改善了方法的选择性，可直接分光光度测定矿石及钢中微量Ｍ     

5‘—硝基水杨基荧光酮胶束增敏分光光度法测定微量钯

于ｐＨ６．７￣７．６的磷酸盐缓冲介质中，溴化十六烷基三甲铵存在下，Ｐｄ（Ⅱ）与５＇－硝基水杨基荧光酮３０ｍｉｎ内反应完全，生成组成比１：２的紫红色配合物。λｍａｘ＝５８２ｎｍ，Δλ＝５６ｎｍ，表观ε为１．０４×１０＾５Ｌ·ｍｏｌ＾－１·ｃｍ＾－１，配合物至少稳定３６ｈ。测Ｐｄ（Ⅱ）的线性范围在０￣０．８０ｍｇ／Ｌ。结合丁二酮肟－氯仿萃取分离，方法可用于试样中微量钯的测定，结果与５－Ｂｒ－ＰＡＤＡＢ     

钪－4，5－二溴苯基荧光酮－CTMAB－吐温－60多元配合物的分光光度法研究

研究结果表明，在混合表面活性剂ＣＴＭＡＢ－吐温－６０存在下的ＰＨ５．７－６．５的缓冲介质中，Ｓｃ（Ⅲ）与４，５－二溴苯基荧光酮形成高灵敏的多元配合物，其ε５９０＝２．２６×１０＾５Ｌ．ｍｏｌ＾－１．ｃｍ＾－１，组成比为：Ｓｃ：ＤＢＰＦ：ＣＴＭＡＢ＝１：２：４。采用混合表面活性剂使增溶增敏作用更为显著，并加速了显色反应，增强了配合物的稳定性。而Ｎａ２ＳＯ４的加入能显著地提高体系的灵敏度，Ｓｃ量在０－     

TritonX—100—5—Br—PADAP光度法测定铜和镍

研究了非离子型表面活性剂ＴｒｉｔｏｎＸ－１００存在下,用５－Ｂｒ－ＰＡＤＡＰ光度法测定铜镍的方法。结果表明：在ＰＨ９．０的硼砂缓冲介质中,５－Ｂｒ－ＰＡＤＡＰ与铜和镍生成紫红色络合物,λｍａｘ＾Ｃｕ＝５７５ｎｍ,εＣｕ＝１．０４×１０＾５Ｌ·ｍｏｌ＾－１·ｃｍ＾－１,λｍａｘ＾Ｎｉ＝５７５ｎｍ,εＮｉ＝１．１４×１０＾５Ｌ·ｍｏｌ＾－１·ｎｍ＾－１。铜和镍的质量浓度分别在０￣５６０μｇ／Ｌ和０￣５     

2—[2—（5—甲基苯并噻唑）偶氮]—5—二乙氨基苯甲酸的离解平衡及其与？…

研究了新显色剂２－「２－（５－甲基苯并噻唑）偶氮」－５－二乙氨基苯甲酸（５－Ｍｅ－ＢＴＡＥＢ）的离解平衡及与Ｆｅ＾２＋形成配合物的条件。在十二烷基硫酸钠的存在下,５－Ｍｅ－ＢＴＡＥＢ与Ｆｅ＾２＋形成稳定的蓝紫色２：１配合物,其最大吸收波长为６４０ｎｍ,表观摩尔吸光系数为１．０３＊１０＾５Ｌ．ｍｏｌ＾－１．ｃｍ＾－１。Ｆｅ＾２＋的质量浓度在０－４８０μｇ／Ｌ时服比尔定律。方法用于部级铝合金标样中微量     

Niobium and Tantalum Concentrations in NIST SRM 610 Revisited

Niobium and Ta concentrations in MPI‐DING and USGS (BCR‐2G, BHVO‐2G, BIR‐1G) silicate rock glasses and the NIST SRM 610–614 synthetic soda‐lime glasses were determined by 193 nm ArF excimer laser ablation and quadrupole ICP‐MS. Measured Nb and Ta values of MPI‐DING glasses were found to be consistently lower than the recommended values by about 15% and 25%, respectively, if calibration was undertaken using commonly accepted values of NIST SRM 610 given by Pearce et al. Analytical precision, as given by the 1 s relative standard deviation (% RSD) was less than 10% for Nb and Ta at concentrations higher than 0.1 μg g^?1. A significant negative correlation was found between logarithmic concentration and logarithmic RSD, with correlation coefficients of ‐0.94 for Nb and ‐0.96 for Ta. This trend indicates that the analytical precision follows counting statistics and thus most of the measurement uncertainty was analytical in origin and not due to chemical heterogeneities. Large differences between measured and expected Nb and Ta in glasses GOR128‐G and GOR132‐G are likely to have been caused by the high RSDs associated with their very low concentrations. However, this cannot explain the large differences between measured and expected Nb and Ta in other MPI‐DING glasses, since the differences are normally higher than RSD by a factor of 3. Count rates for Nb and Ta, normalised to Ca sensitivity, for the MPI‐DING, USGS and NIST SRM 612–614 glasses were used to construct calibration curves for determining NIST SRM 610 concentrations at crater diameters ranging from 16 (im to 60 μm. The excellent correlation between the Nb/Ca_1μgg‐1 signal (Nb represents the Nb signal intensity; Ca_{1μg g‐1} represents the Ca sensitivity) and Nb concentration, and between the Ta/Ca_{1μg g‐1} signal (where Ta represents the Ta signal intensity; Ca_{1μg g‐1} represents the Ca sensitivity) and Ta concentration (R²= 0.9992–1.00) in the various glass matrices suggests that matrix‐dependent fractionation for Nb, Ta and Ca was insignificant under the given instrumental conditions. The results confirm that calibration reference values of Nb and Ta in NIST SRM 610 given by Pearce et al. are about 16% and 28% lower, respectively. We thus propose a revision of the preferred value for Nb from 419.4 ± 57.6 μg g^?1 to 485 ± 5 μg g^?1 (1 s) and for Ta from 376.6 ± 77.6 μg g^?1 to 482 ± 4 μg g^?1 (Is) in NIST SRM 610. Using these revised values for external calibration, most of the determined average values of MPI‐DING, USGS and NIST SRM 612–614 reference glasses agree within 3% with the calculated means of reported reference values. Bulk analysis of NIST SRM 610 by standard additions using membrane desolvation ICP‐MS gave Nb = 479 ± 6 μg g^?1 (1 s) and Ta = 468 ± 7 μg g^?1 (1 s), which agree with the above revised values within 3%.     

Determination of the Trace Refractory Elements V, Nb and Ta in Environmental Samples by ICP-MS After Separation and Preconcentration with Nanometre-Sized Alumina Microcolumns Following Chemical Modification by Gallic Acid

Nanometre-sized alumina was chemically modified with gallic acid (GA) and used as a solid phase adsorption material for the determination of trace amounts of V, Nb and Ta in natural water, soil and stream sediment samples by inductively coupled plasma-mass spectrometry. The effects of pH, sample flow rate and volume, elution solution and interfering ions on the recovery of the analytes were investigated. The results showed that V, Nb and Ta could be adsorbed at pH 4.0 and recovered with 1 ml of 2.0 mol l^-1 HCl. Under optimised conditions, the adsorption capacity of GA-modified nanometre-sized Al₂O₃ was found to be 7.0, 8.9, 13.3 mg g^-1 for V, Nb and Ta, respectively. The limits of detection were as low as 0.25, 0.24 and 0.66 ng l^-1 for V, Nb and Ta, respectively with a concentration factor of fifty. The recovery of V, Nb and Ta for spiked water samples was between 85.7 and 116%. The developed method has also been applied to the determination of trace V, Nb and Ta in soil and stream sediment certified materials, and the determined values were in a good agreement with the certified values.     

K比例H点标准加入吸光光度法同时测定矿样中铌和钽

从样品分解方法入手,探讨了最佳测试条件。用盐酸-氟化氢铵-硝酸-高氯酸溶解试样,在10%的盐酸介质中,用火焰原子吸收光谱仪于波长328.1 nm处,以空气-乙炔火焰测定铅精粉中的银量,克服了用铅析或灰吹法测定的步骤冗长等缺点。用铅精粉国家一级标准物质GBW 07167分析验证,测定结果与标准值吻合。方法精密度(RSD,n=12)为2.2%~4.3%,方法检出限为1.2μg/g。方法分析快速,简单。     

丹宁棉分离富集—发射光谱法同时测定地质样品中微量铌钽锆铪

采用丹宁棉对地质样品溶液中的铌、钽、锆、铪进行分离富集，将写信后的丹宁棉在600℃灼烧30min，灰分用发射光谱法同时测定四元素。检出限与通常的发射光谱法相比降低约2个数量级，经国家级标准物质检验，结果与标准值相符，精密度试验，各元素的RSD（n＝20）为2.6％－7.9％。     

常压混酸溶矿一电感耦合等离子体发射光谱法测定铌钽

混酸溶解矿石样品,在酒石酸介质中,用电感耦合等离子体发生光谱法(ICP-AES)测定溶液中的铌钽。该方法ρ(Nb₂O₅)和ρ(Ta₂O₅)在0～20 μg/mL时,铌钽原子发射光谱强度与浓度呈良好的直线关系,Nb、Ta标准曲线相关系数尺分别为0.999 9和0.999 7。检出限分别为0.023 μg/mL和0.072 μg/mL。本方法测定标准样品,测定值与认定值相符。对实际样品分析,Nh、Ta的相对标准偏差(n=6)分别为0.42％～2.3％和1.8％～3.3％,加标回收率均为97％～103％,适合地质找矿、选冶等领域的样品测试。     

Determination of Forty Two Major and Trace Elements in USGS and NIST SRM Glasses by Laser Ablation-Inductively Coupled Plasma-Mass Spectrometry

Forty two major (Na, Mg, Ti and Mn) and trace elements covering the mass range from Li to U in three USGS basalt glass reference materials BCR‐2G, BHVO‐2G and BIR‐1G were determined using laser ablation‐inductively coupled plasma‐mass spectrometry. Calibration was performed using NIST SRM 610 in conjunction with internal standardisation using Ca. Determinations were also made on NIST SRM 612 and 614 as well as NIST SRM 610 as unknown samples, and included forty five major (Al and Na) and trace elements. Relative standard deviation (RSD) of determinations was below 10% for most elements in all the glasses under investigation. Consistent exceptions were Sn and Sb in BCR‐2G, BHVO‐2G and BIR‐1G. For BCR‐2G, BHVO‐2G and BIR‐1G, clear negative correlations on a logarithmic scale exist between RSD and concentration for elements lower than 1500 μg g^‐1 with logarithmic correlation coefficients between ‐0.75 and ‐0.86. There is also a clear trend of increasing RSD with decreasing concentration from NIST SRM 610 through SRM 612 to SRM 614. These suggest that the difference in the scatter of apparent element concentrations is not due to chemical heterogeneity but reflects analytical uncertainty. It is concluded that all these glasses are, overall, homogeneous on a scale of 60 μm. Our first results on BHVO‐2G and BIR‐1G showed that they generally agreed with BHVO‐2/BHVO‐1 and BIR‐1 within 10% relative. Exceptions were Nb, Ta and Pb in BHVO‐2G, which were 14‐45% lower than reference values for BHVO‐2 and BHVO‐1. Be, Ni, Zn, Y, Zr, Nb, Sn, Sb, Gd, Tb, Er, Pb and U in BIR‐1G were also exceptions. However, of these elements, Be, Nb, Sn, Sb, Gd, Tb, Pb and U gave results that were consistent within an uncertainty of 2s between our data and BIR‐1 reference values. Results on NIST SRM 612 agreed well with published data, except for Mg and Sn. This was also true for elements with m/z 85 (Rb) in the case of NIST SRM 614. The good agreement between measured and reference values for Na and Mg in BCR‐2G, BHVO‐2G and BIR‐1G, and for Al and Na in NIST SRM 610, 612 and 614 up to concentrations of at least several weight percent (which were possible to analyse due to the dynamic range of 10⁸) indicates the suitability of this technique for major, minor and trace element determinations.     

Determination of Rare Earth Elements, Y, Th, Zr, Hf, Nb and Ta in Geological Reference Materials G-2, G-3, SCo-1 and WGB-1 by Sodium Peroxide Sintering and Inductively Coupled Plasma-Mass Spectrometry

Data are reported for rare earth elements (REE), Y, Th, Zr, Hf, Nb and Ta in four geological reference materials using sodium peroxide (Na₂O₂) sintering and inductively coupled plasma-mass spectrometry. The described procedure was used by students during their thesis work. A compilation of their reference material data acquired over one year of laboratory work demonstrates the ease and reliability of the method and the high reproducibility of the analytical results. Relative standard deviations of up to thirty six measurements of one reference material were lower than 5% for Y and the REE. Reproduciblities of Zr, Hf, Nb, Ta and Th were higher at between 5% and 10%, and can be attributed to the inhomogeneous distribution of zircon and other trace mineral phases and uncorrected drift effects. The concentration data are compared to reference and literature values and demonstrate that the procedure is also accurate. New data on G-3 show some systematic deviations from G-2, which are statistically significant.     

HFSE systematics of rutile-bearing eclogites: New insights into subduction zone processes and implications for the earth’s HFSE budget

The depleted mantle and the continental crust are generally thought to balance the budget of refractory and lithophile elements of the Bulk Silicate Earth (BSE), resulting in complementary trace element patterns. However, the two high field strength elements (HFSE) niobium and tantalum appear to contradict this mass balance. All reservoirs of the silicate Earth exhibit subchondritic Nb/Ta ratios, possibly as a result of Nb depletion.In this study a series of nineteen orogenic MORB-type eclogites from different localities was analyzed to determine their HFSE concentrations and to contribute to the question of whether subducted oceanic crust could form a hidden reservoir to account for the mass imbalance of Nb/Ta between BSE and the chondritic reservoir. Concentrations of HFSE were analyzed with isotope dilution (ID) techniques. Additionally, LA-ICPMS analyses of clinopyroxene, garnet and rutile have been performed. Rutile is by far the major host for Nb and Ta in all analyzed eclogites. However, many rutiles revealed zoning in Nb/Ta ratios, with cores being higher than rims. Accordingly, in situ analyses of rutiles have to be evaluated carefully and rutile cores do not necessarily reflect a bulk rock Nb and Ta composition, although over 90% of these elements reside in rutile.The HFSE concentration data in bulk rocks show that the orogenic eclogites have subchondritic Nb/Ta ratios and near chondritic Zr/Hf ratios. The investigated eclogites show neither enrichment of Nb compared to similarly incompatible elements (e.g. La), nor fractionation of Nb/Ta ratios relative to MOR-basalts, the likely precursor of these rocks. This indicates that during the conversion of the oceanic crust to eclogites in most cases, (1) HFSE and REE have similar mobility on average, possibly because both element groups remain in the down going slab, and (2) no significant fractionation of Nb/Ta occurs in subducted oceanic crust. With an average Nb/Ta ratio of 14.2 ± 1.4 (2s.e.), the investigated eclogites cannot balance the differences between BSE and chondrite. Additionally, as their average Nb/Ta is indistinguishable from the Nb/Ta of MORB, they are also an unlikely candidate to balance the potentially small differences in Nb/Ta between the continental crust and the mantle.     

Primary and secondary niobium mineral deposits associated with carbonatites

This work reviews the character and origin of primary and supergene economic deposits of niobium associated with carbonatites. The Brazilian supergene deposits account for about 92% of the total worldwide production of Nb, with the primary St. Honoré carbonatite and other sources accounting for only for 7 and 1%, respectively. The emphasis of the review is upon the styles of Nb mineralization and the geological factors which lead to economic concentrations of Nb-bearing minerals. Primary economic deposits of Nb are associated principally with carbonatites found in diverse types of plutonic alkaline rock complexes. Primary magmas are principally those of the melilitite, nephelinite and aillikite clans. Although many primary niobium deposits are associated with carbonatites, ijolites and syenites in the same alkaline complexes can also contain significant Nb mineralization in the form of niobian titanite and diverse Nb–Zr-silicates (marianoite-wöhlerite); these potential sources of Nb have not as yet been explored or exploited. Primary Nb deposits can be regarded as large tonnage, low grade (typically < 1 wt.% Nb₂O₅) disseminated ore deposits. Niobium is hosted principally by diverse Na–Ca–U-pyrochlores, ferrocolumbite and fersmite. Every actual, and potential, primary Nb deposit is unique with respect to the varieties of pyrochlore present; extent of replacement by other minerals; and degree of alteration by deuteric/hydrothermal fluids. Within a given occurrence individual petrographically-defined units of carbonatite contain distinct suites of pyrochlore. Bulk rock analysis for Nb gives no indication of the style of mineralization and provides no information of use regarding beneficiation of the ore. Evaluation of any Nb deposit requires extensive definition drilling and detailed mineralogical studies. Primary Nb deposits result from the early crystallization of Nb-bearing minerals in magma chambers followed by crystal fractionation, magma mixing, and redistribution of Nb-minerals by density currents. Supergene Nb deposits occur in laterites formed by extensive weathering of primary carbonatites. The process results in the decomposition of apatite and magnetite, removal of soluble carbonates and physical concentration of resistant primary pyrochlore. Intense lateritization results initially in the replacement of primary pyrochlores by supergene, commonly Ba, Sr, K or Pb-bearing pyrochlores, and ultimately complete decomposition of pyrochlore and formation of Nb-bearing rutile, brookite, and anatase. The Nb contents of the laterites can be enriched up to 10 times or more above those of the primary carbonatite. Commonly, pyrochlores in laterites are fine grained and intimately intergrown with hematite, goethite and minerals of the crandallite group. The different styles of mineralization of primary and secondary Nb deposits require different methods of ore beneficiation.