感耦等离子体发射光谱法测定纯氧化镧中稀土和非稀土杂质

研究了用感耦等离子体发射光谱（ＩＣＰ－ＡＥＳ）测定纯氧化镧中Ｃｅ，Ｐｒ，Ｎｄ，Ｓｍ，Ｙ，Ｆｅ，Ａｌ，Ｃａ，Ｍｇ和Ｓｉ１０个杂质元素的方法。考察了基体镧的光谱干扰，共存元素间光谱干扰及校正方法，方法检出限为０．０００５－０．０３９μｇ／ｍｌ；标准加入量１μｇ／ｍｌ时，回收率为９５％－１０６％；１０μｇ／ｍｌ的标准溶液，测定１０次，ＲＳＤ为０．２４％－１．０１％。方法简单，快速，不震分离富集，适用于氧     

微波诱导等离子体原子发射光谱法测定汞的研究

研究了以常压低功率氩微波诱导等离子体为激发源的原子发射光谱测定Hg的方法。采用超声雾化、水冷凝、浓H_2SO_4吸收去溶的进样方法,考察了微波前向功率、载气流速、KCl和NH_4Cl浓度、酸度等因素对Hg发射强度的影响。方法已用于试样分析。     

Enhanced ion acoustic fluctuations and ion outflows

A number of observations showing enhanced ion acoustic echoes observed by means of incoherent scatter radars have been reported in the literature. The Received power is extremely enhanced by up to 1 or 2 orders of magnitude above usual values, and it is mostly contained in one of the two ion acoustic lines. This spectral asymmetry and the intensity of the received signal cannot be resolved by the standard analysis procedure and often causes its failure. As a result, and in spite of a very clear spectral signature, the analysis is unable to fit the plasma parameters inside the regions of ion acoustic turbulence. We present European Incoherent Scatter radar (EISCAT) observations of large ion outflows associated with the simultaneous occurrence of enhanced ion acoustic echoes. The ion fluxes can reach 10¹⁴ m^–2 s^–1 at 800 km altitude. From the very clear spectral signatures of these echoes, a method is presented to extract estimates of the electron temperature and the ion drift within the turbulent regions. It is shown that the electron gas is strongly heated up to 11 000 K. Also electron temperature gradients of about 0.02 K/m exist. Finally, the estimates of the electron temperature and of the ion drift are used to study the possible implications for the plasma transport inside turbulent regions. It is shown that strong electron temperature gradients cause enhancement of the ambipolar electric field and can account for the observed ion outflows.     

Global Substorm Cycle: What can the models tell us?

Magnetospheric substorms represent the basic dynamic process in the coupled solar wind -- magnetosphere -- ionosphere system. Recent satellite missions have considerably advanced our means to monitor this vast environment. These observations are interpreted in the context of a hierarchy of models: Global MHD simulations and various techniques of nonlinear physics are used to characterize the large-scale features, whereas microphysical models are used to study the small-scale processes. Empirical models are described in order to address questions that involve meso-scale or multi-scale phenomena. We discuss some of the recent observations and relate those to new advancements in various modeling techniques.     

萃取色谱富集—等离子体质谱测定海水中的超痕量稀土

用Ｐ５０７萃淋树脂为固定相，ＨＣｌ为流动相，在小柱（７ｍｍ×１０ｍｍ）上试验研究了海水中稀土元素（ＲＥＥ）的分离富集条件以及Ｂａ的干扰消除方法。以５．０ｍＬ／ｍｉｎ的流速大体积（１Ｌ海水）上柱，用５０ｍＬ６ｍｏｌ／ＬＨＣｌ以２．５ｍＬ／ｍｉｎ的流速洗脱，实现了海水中超痕量稀土的分离富集，建立了一个ＩＣＰ＿ＭＳ测定海水中超痕量稀土的新方法。方法的检测限为０．０５～２．６２ｎｇ／Ｌ，标准回收率大于９８％，精密度（ＲＳＤ，ｎ＝７）小于５％。     

The Inner Magnetosphere: A Review

This paper addresses research achievements during roughly the period 1991–1993 pertaining to the inner magnetosphere including the radiation belts, plasmasphere, and ring current region. It also addresses issues concerning the magnetic fields, electrical currents, and particle precipitation properties that relate to this region of the solar-terrestrial system. Recent analysis and modeling of magnetospheric substorms and geomagnetic storms affecting the inner edge of the plasma sheet are discussed and the regions from the geostationary orbit inward toward the Earth are examined in light of new observational and theoretical tools.Presented at the 7th Scientific Assembly International Association of Geomagnetism and Aeronomy Buenos Aires, Argentina 8–20 August 1993.     

西太平洋海山富钴结壳稀土元素(REE)组成原位LA-ICPMS测定

利用激光剥蚀电感耦合等离子体质谱(LA-ICPMS)微区原位分析方法,对采自西太平洋海山具完整三层结构的富钴结壳样品进行了稀土元素(REE)含量测定,结果表明, 虽然均产于西太平洋海山且均具有明显的三层结构,富钴结壳化学组成受地理位置和沉积环境影响很大。绝大多数西太平洋富钴结壳具有高ΣREE、高LREE/HREE、δCe正异常和δEu基本无异常或微弱正异常的特点, 显示它们主要由正常海水沉积形成。结壳不同层圈之间REE组成有较大的区别, 其原因主要在于其形成环境和矿物组成不同。样品0327稀土元素总量(∑REE)由亮煤层到疏松层到外层逐渐升高,且亮煤层δCe和Y/Ho变化非常大,最大值分别为38.61和105.5,显示该层生长环境较为氧化且相对动荡,而样品0346中三层结构的∑REE都非常高,且变化趋势与0327正好相反,从亮煤层到致密层∑REE有降低的趋势。 亮煤层形成时海水相对较氧化的环境有利于铁锰氧化物的形成和Ce⁴⁺等稀土元素的吸附,导致其中ΣREE较疏松层和外层为高,而后期磷酸盐化导致REE元素的迁移和亏损。在结壳生长剖面上,由最外层到疏松层和亮煤层,δCe呈明显上升趋势,且变化范围趋大,说明该结壳所处的海水环境在由老至新的生长过程中由相对动荡和氧化变为相对平静和还原。     

激光进样等离子体质谱技术及其在地球科学中的应用

对激光进样等离子体质谱固体分析新技术进行了评述,包括这一技术的性能特点、仪器结构和进展概况、有关参数、分析理论、样品制备及其在地球科学中的应用。引用主要文献４１篇。     

Zinc Isotopic Compositions of NIST SRM 683 and Whole‐Rock Reference Materials

In this study the homogeneity of the zinc isotopic composition in the NIST SRM 683 reference material was examined by measuring the Zn isotopic signature in microdrilled sample powders from two metal nuggets. Zinc was purified using AG MP‐1M resin and then measured by MC‐ICP‐MS. Instrumental mass bias was corrected using the “sample‐standard bracketing” method and empirical external normalisation with Cu doping. After evaluating the potential effects of varying acid mass fractions and different matrices, high‐precision Zn isotope data were obtained with an intermediate measurement precision better than ± 0.05‰ (δ⁶⁶Zn, 2s) over a period of 5 months. The δ⁶⁶Zn_JMC‐Lyon mean values of eighty‐four and fourteen drilled powders from two nuggets were 0.11 ± 0.02‰ and 0.12 ± 0.02‰, respectively, indicating that NIST SRM 683 is a good isotopic reference material with homogeneous Zn isotopes. The Zn isotopic compositions of seventeen rock reference materials were also determined, and their δ⁶⁶Zn values were in agreement with most previously published data within 2s. The δ⁶⁶Zn values of most of the rock reference materials analysed were in the range 0.22–0.36‰, except for GSP‐2 (1.07 ± 0.06‰, n = 12), NOD‐A‐1 (0.96 ± 0.03‰, n = 6) and NOD‐P‐1 (0.78 ± 0.03‰, n = 6). These comprehensive data should serve as reference values for quality assurance and interlaboratory calibration exercises.     

Forty‐Nine Major and Trace Element Concentrations Measured in Soil Reference Materials NIST SRM 2586, 2587, 2709a, 2710a and 2711a Using ICP‐MS and Wavelength Dispersive‐XRF

Excellent agreement was noted in the concentration of major and trace elements in five NIST (National Institute for Science and Technology) soil reference materials (NIST SRM 2586, 2587, 2709a, 2710a and 2711a) between measurement results from wavelength dispersive‐XRF and ICP‐MS from two independent laboratories, and NIST certificate of analysis and literature data. We describe the variability in concentrations of up to forty‐nine elements (plus loss on ignition) and provide values for up to twenty‐one elements previously uncharacterised by NIST in these soil RMs. The additional characterisation provided in this investigation can be utilised to reduce the measurement bias of custom calibration routines and improve the quality of control checks developed using these NIST RMs.