玩具业中重金属的等离子体发射光谱分析     

LEE Davidowski  ZOE Grosser  LAURA Thompson 《岩矿测试》2009,28(2):203-205

为了支持玩具业,许多实验室需要分析各种复杂基体中的金属含量。人们关心的主要元素是铅,但很多其他有毒元素也具有潜在的威胁,尤其对于儿童。这些重金属元素包括锑、砷、钡、镉、铬、硒、汞和铅,累积在人体中将产生不利的影响。一些塑料和木制玩具,特别是表面色彩鲜艳的玩具被证实含有更高水平的铅和其他元素,儿童因接触易摄入,相关法规对产品表面含有这些元素的材料作了一些限制。为了保证玩具和其他物品的生产、流通和销售,有必要检测其中的重金属含量。不同的管理机构对各类样品中的元素提供了限量要求。在玩具安全性的欧洲标准EN71第3部分(已纳入ISO8124-3),其中在“特定元素的迁移”一节给出了玩具材料中元素迁移的  相似文献   

Intercomparison of the LASCO-C2, SECCHI-COR1, SECCHI-COR2, and Mk4 Coronagraphs     

Richard A. Frazin  Alberto M. Vásquez  William T. Thompson  Russell J. Hewett  Philippe Lamy  Antoine Llebaria  Angelos Vourlidas  Joan Burkepile 《Solar physics》2012,280(1):273-293

In order to assess the reliability and consistency of white-light coronagraph measurements, we report on quantitative comparisons between polarized brightness [pB] and total brightness [B] images taken by the following white-light coronagraphs: LASCO-C2 on SOHO, SECCHI-COR1 and -COR2 on STEREO, and the ground-based MLSO-Mk4. The data for this comparison were taken on 16?April 2007, when both STEREO spacecraft were within 3.1^° of Earth??s heliographic longitude, affording essentially the same view of the Sun for all of the instruments. Due to the difficulties of estimating stray-light backgrounds in COR1 and COR2, only Mk4 and C2 produce reliable coronal-hole values (but not at overlapping heights), and these cannot be validated without rocket flights or ground-based eclipse measurements. Generally, the agreement between all of the instruments?? pB values is within the uncertainties in bright streamer structures, implying that measurements of bright CMEs also should be trustworthy. Dominant sources of uncertainty and stray light are discussed, as is the design of future coronagraphs from the perspective of the experiences with these instruments.  相似文献   

Using a fluvial archive to place extreme flood sediment (dis)connectivity dynamics in context of a longer-term record     

Kirstie Fryirs  Chris Thompson  Damian Gore 《国际泥沙研究》2022,37(4):447-456

The aim of this study was to establish the source and provenance of sediments deposited in a large floodplain sink during extreme floods in the Lockyer Creek catchment, Australia, in 2011 and 2013. We place the sediment source patterns in context of the longer-term record to determine whether coarse-grained sediment sources (i.e., very fine sand to very coarse sand) and the spatio-temporal pattern of (dis)connectivity have changed over time. We do this by matching the geochemical properties and age structure of a sediment profile located in a downstream floodplain sink to the elemental composition of source sediments. One hundred and fifty-seven sediment samples from 20 sites across the catchment are analysed using X-ray fluorescence (XRF) spectrometry to compare the elemental ratio composition of the downstream floodplain sink to its source materials. We use Optically Stimulated Luminescence (OSL) dating to determine the age structure of the sediments in the floodplain sink. The northern tributaries and parts of the Lockyer River trunk stream are the primary sources of coarse sediment. These areas are connected (coupled) to the lower trunk stream and floodplain sediment sink. Southern tributaries are largely disconnected (decoupled) and supply little sediment to the floodplain sediment sink. This pattern of sediment source contribution has remained similar over the last 6.8 ka at least. Sediment sources as observed in the 2011 flood have predominated over the mid-late Holocene whilst those in the 2013 flood are rare.  相似文献   

Time – Distance Analysis of the Emerging Active Region NOAA 10790     

S. Zharkov  M. J. Thompson 《Solar physics》2008,251(1-2):369-380

We investigate the emergence of Active Region NOAA 10790 by means of time?–?distance helioseismology. Shallow regions of increased sound speed at the location of increased magnetic activity are observed, with regions becoming deeper at the locations of sunspot pores. We also see a long-lasting region of decreased sound speed located underneath the region of the flux emergence, possibly relating to a temperature perturbation due to magnetic quenching of eddy diffusivity, or to a dense flux tube. We detect and track an object in the subsurface layers of the Sun characterised by increased sound speed which could be related to emerging magnetic-flux and thus obtain a provisional estimate of the speed of emergence of around 1 km?s^?1.  相似文献   

Editors' note: Astron. Nachr. 5/2008     

S. J. Jimnez Reyes  D. R. Reese  M. J. Thompson 《Astronomische Nachrichten》2008,329(5):439-439

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Geochemistry and provenance of the Turquoise Bluff Slate,northeastern Tasmania: tectonic significance     

R. F. Berry  K. Goemann  J. Thompson  S. Meffre  R. Bottrill 《Australian Journal of Earth Sciences》2019,66(2):227-246

The Ordovician Turquoise Bluff Slate in northeastern Tasmania is a 2?km-thick sequence of deep-marine siliceous black slates. It is dominated by meta-siltstones with bimodal grainsize distributions typical of turbidite T_E-1 and T_E-2 facies. The slates have high SiO₂ indicating they are hemipelagites. The high Ba and V indicate they were deposited in an anoxic environment associated with high oceanic productivity. All these features are common in muddy turbidites. U–Th–Pb dating of detrital monazite and authigenic xenotime in the slates supports previous evidence that the dominant cleavage, in this unit, formed during the Benambran Orogeny. The whole-rock composition of the slates is similar to black slates in the Adaminaby Group, NSW. A review of Paleozoic whole-rock compositions from the Lachlan Orogen confirms they all have trace element contents similar to average Australian shale. However, there are subtle differences in composition. The Turquoise Bluff Slate and other Mathinna Supergroup rocks from the Eastern Tasmania Terrane have higher average Cr content than similar age turbidites from Victoria and NSW. This probably reflects a small contribution from Tasmania Cambrian ultramafic rocks in the provenance. If this were correct, northeastern Tasmania was closer to western Tasmania in the Paleozoic than other provinces of the Lachlan Orogen, southeastern Australia. Other subtle features of the whole-rock composition of Paleozoic sedimentary rocks from the Lachlan Orogen indicate it may be possible to recognise provincial variations in composition that will provide new constraints on tectonic models of southeastern Australia.  相似文献   

A search for posteclipse brightening of Io in 1973. I     

R.L. Millis  D.T. Thompson  B.J. Harris  P. Birch  R. Sefton 《Icarus》1974,23(3):425-430

Eight eclipse reappearances of the innermost Galilean satellite, Io, were observed during the fall of 1973. The measurements were made using photometers specially designed to cope with the problem of scattered light from Jupiter. Posteclipse brightening of Io was not detected and, if present, was less than our estimated detection threshold of about 0.02 mag.  相似文献   

A Review Of The National Science Foundation Short Course On Models Of Urban Spatial Structure And Ecology,June 29–July 16, 1971.     

Donald G. Janelle  Bryan Thompson 《The Professional geographer》1972,24(1):43-44

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Spatial Pair-Copula Modeling of Grade in Ore Bodies: A Case Study     

G. Nishani Musafer  M. Helen Thompson  E. Kozan  R. C. Wolff 《Natural Resources Research》2017,26(2):223-236

A real-world mining application of pair-copulas is presented to model the spatial distribution of metal grade in an ore body. Inaccurate estimation of metal grade in an ore reserve can lead to failure of a mining project. Conventional kriged models are the most commonly used models for estimating grade and other spatial variables. However, kriged models use the variogram or covariance function, which produces a single average value to represent the spatial dependence for a given distance. Kriged models also assume linear spatial dependence. In the application, spatial pair-copulas are used to appropriately model the non-linear spatial dependence present in the data. The spatial pair-copula model is adopted over other copula-based spatial models since it is better able to capture complex spatial dependence structures. The performance of the pair-copula model is shown to be favorable compared to a conventional lognormal kriged model.  相似文献   

Making ends meet, in the household and on the planet     

Karl Dake  Michael Thompson 《GeoJournal》1999,47(3):417-424

Policy-making in relation to sustainable development is usually at the national (or, in relation to climate change, the global) level, yet the consumption it seeks to modify takes place at the household level. If households all ‘made ends meet’ in the same way then the much-relied upon notion of per capita consumption would be valid and we could rely on ‘top-down’ modelling to guide policy. Cultural Theory, however, predicts that there are five socially viable ways of making ends meet, and that all of them will be found (in varying proportions) within any nation. This prediction has been tested on a sample of 220 British households and shown to be well supported. Top-down modelling, it is argued, has to give way to a constructive interplay between the reflexive policy-maker and a plurally responsive citizenry. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献