金昌市铜镍矿区周围土壤中重金属的迁移特征

对金昌矿区不同区域土壤5~20 cm层中重金属各化学形态及活性态的迁移行为进行了研究,结果表明：土壤中重金属不同化学形态迁移率不同,弱酸提取态、可还原态、可氧化态和残渣态平均迁移率分别为0.13、0.51、0.30和0.54。重金属总量和活性态（包括弱酸提取态、可还原态、可氧化态）迁移率也表现出很大差异,尾矿区土壤Cr总量迁移率较高为0.65,而其活性态迁移率较低为0.26,Ni与Cr迁移特征完全相反,总量迁移率为0.26,而活性态迁移率为0.67;农田土壤中Pb总量迁移率低而活性态迁移率高,Ni与Zn特征相似,总量迁移率高而活性态迁移率相对较低;大棚地土壤中重金属迁移率均较低,Cu和Ni活性态几乎未发生向下迁移。可见,重金属的迁移与其化学形态分布关系密切,与重金属总量的迁移率相比,活性态迁移率能够更有效地反映出土壤中重金属的迁移特征和潜在危害性。     

QoS感知的多任务遥感信息服务优化组合非合作博弈模型

提出了QoS感知的多任务服务优化组合非合作博弈模型,准确刻画了不同任务之间的竞争关系,在此基础上设计了顾及QoS的遥感信息服务优化组合反应函数,为求解遥感信息服务优化组合奠定理论基础。理论和实验分析表明,该模型有利于减少任务并发时的资源冲突,最大化所有任务的平均效用。     

Coupling photochemistry with haze formation in Titan's atmosphere, Part II: Results and validation with Cassini/Huygens data

The new one-dimensional radiative-convective/photochemical/microphysical model described in Part I is applied to the study of Titan's atmospheric processes that lead to haze formation. Our model generates the haze structure from the gaseous species photochemistry. Model results are presented for the species vertical concentration profiles, haze formation and its radiative properties, vertical temperature/density profiles and geometric albedo. These are validated against Cassini/Huygens observations and other ground-based and space-borne measurements. The model reproduces well most of the latest measurements from the Cassini/Huygens instruments for the chemical composition of Titan's atmosphere and the vertical profiles of the observed species. For the haze production we have included pathways that are based on pure hydrocarbons, pure nitriles and hydrocarbon/nitrile copolymers. From these, the nitrile and copolymer pathways provide the stronger contribution, in agreement with the results from the ACP instrument, which support the incorporation of nitrogen in the pyrolized haze structures. Our haze model reveals a new second major peak in the vertical profile of haze production rate between 500 and 900 km. This peak is produced by the copolymer family used and has important ramifications for the vertical atmospheric temperature profile and geometric albedo. In particular, the existence of this second peak determines the vertical profile of haze extinction. Our model results have been compared with the DISR retrieved haze extinction profiles and are found to be in very good agreement. We have also incorporated in our model heterogeneous chemistry on the haze particles that converts atomic hydrogen to molecular hydrogen. The resultant H₂ profile is closer to the INMS measurements, while the vertical profile of the diacetylene formed is found to be closer to that of the CIRS profile when this heterogenous chemistry is included.     

泉州城市表层土壤重金属的赋存形态及污染评价

本文采用改进的BCR连续提取法研究泉州市区表层土壤中17种重金属的形态分布特征,并运用地积累指数Igeo法、潜在生态危害指数法、次生相与原生相分布比值法(RSP)评价土壤中重金属元素的潜在生态危害。结果表明,Li,Ti,Fe,Sc,V,As,Sb,Sn主要以残渣态存在;Cr,Ni,Cu,Zn,Bi在可氧化态中占有大比例,但仍以残渣态为主;Pb以可还原态为主;Mn,Cd,Co在可还原态和残渣态中占有较大比例。根据地累积指数法和RSP,泉州土壤受到不同程度的Sc,Co,Ni,Cu,Cd,Sb,Pb污染;潜在生态危害指数表明泉州市城区受到轻微生态危害。     

全新世岱海流域化学风化及其对气候事件的响应

通过对岱海 12.08 m沉积岩芯 210Pb和 AMS- 14C精确定年及地球化学、物理指标的综合分析,重建了包括 8.2 ka冷期、中世纪暖期 (MWP)和小冰期 (LIA)等典型气候事件在内的全新世以来所经历的化学风化及其环境演化过程.全新世早-中期 (9.0～ 3.5 ka),岱海流域处于温暖湿润气候环境,主要环境特征表现为流域化学风化显著增强、生物生产力逐步提高、湖泊水位大幅度抬升.在 7.90～ 8.25 ka期间存在一次冷气候事件,其发生时间与来自湖沼、海洋、生物组合和极地冰芯等在内的全球环境记录基本一致,具体表现为流域化学风化减弱、湖泊生产力降低以及湖泊水位下降. 2.5 ka以来,岱海沉积物中环境指标的显著变化,表明进入气候波动更频繁的新冰期.岱海沉积物中的指标变化也展示了本世纪以来的气候增暖过程,但其化学风化强度还没有达到 MWP的程度.     

喜马拉雅珠峰地区冬季大气气溶胶化学组分及光学特征

为了研究喜马拉雅山北坡冬季大气气溶胶化学组分、光学特征及来源,2017年11—12月在珠穆朗玛峰站(QOMS)共采集22个PM2.5样品.结果显示:PM2.5中包括水溶性离子(WSIs)、有机质(OM)、元素碳(EC)在内的所有检测成分,总质量浓度为(3.36±1.06)μg·m-3;有机碳(OC)、元素碳(EC)和水...     

透岩浆流体成矿体系

根据透岩浆流体成矿理论,熔浆体系与含矿流体体系可以看作是两个相互独立的地质体系,它们因相互需要而耦合在一起形成一个复杂的混合体系。当熔浆与流体发生解耦时,可以在不同的边界条件下发生不同类型的成矿作用。因此,可以将透岩浆流体成矿体系进一步划分成正岩浆成矿体系、接触带成矿体系、远程热液成矿体系和火山热液成矿体系。如果熔浆具有很强的流体圈闭能力,所有的含矿流体都将被封存在岩浆体内,并随着岩浆的固结而析出成矿物质,形成正岩浆矿床。当岩浆具有较高的渗透率且含矿流体逸出岩浆体时,如果岩浆的直接围岩具有较强的捕获成矿物质的能力,即发生接触带成矿作用。否则,含矿流体将在岩浆热驱动下远离岩浆体,形成远程热液矿床。如果有利的流体通道直达岩浆体,含矿流体甚至可以喷出地表或其附近,形成火山热液矿床或水底喷流沉积矿床。这种理论分析似乎与许多成矿事实相吻合,可以有效地指导区域成矿预测和矿床勘探。     

Barium Isotopic Compositions in Thirty‐Four Geological Reference Materials Analysed by MC‐ICP‐MS

Measurement of Ba isotope ratios of widely available reference materials is required for interlaboratory comparison of data. Here, we present new Ba isotope data for thirty‐four geological reference materials, including silicates, carbonates, river/marine sediments and soils. These reference materials (RMs) cover a wide range of compositions, with Ba mass fractions ranging from 6.4 to 1900 µg g^?1, SiO₂ from 0.62% to 90.36% m/m and MgO from 0.08% to 41.03% m/m. Accuracy and precision of our data were assessed by the analyses of duplicate samples and USGS rock RMs. Barium isotopic compositions for all RMs were in agreement with each other within uncertainty. The variation of δ^138/134Ba in these RMs was up to 0.7‰. The shale reference sample, affected by a high degree of chemical weathering, had the highest δ^138/134Ba (0.37 ± 0.03‰), while the stream sediment obtained from a tributary draining carbonate rocks was characterised by the lowest δ^138/134Ba (?0.30 ± 0.05‰). Geochemical RMs play a fundamental role in the high‐precision and accurate determination of Ba isotopic compositions for natural samples with similar matrices. Analyses of these RMs could provide universal comparability for Ba isotope data and enable assessment of accuracy for interlaboratory data.     

Changes in the ionic composition of a saline lake,Mar Chiquita,Province of Córdoba,Argentina

Mar Chiquita is the largest water-body in Argentina according to area. This ranges from 2,000 km² in dry periods to 5,000 km² in humid ones. Its very high salinity ranged this century from 200 to 300 g/L, but an increase in the average rainfall in the basin since 1973 has led to a rise in lake level and the dilution of its waters to 78 g/L in 1978 and about 30 g/L in the late 1980s. Ionic strength decreased from 6.61 in 1970 to 0.541 in 1986. The composition of the water also changed, with increases in the proportions of sulphate, calcium and magnesium concentrations. The most important processes taking place in solution are calcite and gypsum equilibrium, formation of clay minerals, and sulphate reduction in the interstitial waters of the bottom sediments. The thermodynamic state of the solutions for different years has been obtained. Results show that the solution shifted from gypsum oversaturation in 1970 to gypsum equilibrium in 1978, and to gypsum undersaturation since 1982. A geochemical simulation of the composition of the solution from its origin from mean tributary composition, following a modified Hardie-Eugster model, has been developed using PHRQPITZ. The results agree with empirical observations.     

辽河盆地东部凹陷原油的碳同位素组成特征

通过对辽河盆地东部凹陷原油的饱和烃、芳烃的碳同位素组成特征、原油同位素类型和单体烃同位素特征进行研究 ,发现整个东部凹陷原油及其组分的碳同位素值偏重 ,指示其源岩有机质中藻类和低等水生生物的贡献较少 ;饱和烃—芳烃的碳同位素值关系揭示东部凹陷大部分原油样品与沙河街组沙三段烃源岩的特征相近 ,而南部和北部地区少数样品表现出负的碳同位素异常 ,与该区中生界源岩样品的接近 ,推测原油中可能混入了中生界来源的油气。南部地区各样品的碳同位素类型曲线和单体烃的碳同位素曲线均相似 ,揭示了两者具相同的油气来源。北部地区各原油样品的单体烃的碳同位素类型曲线间具有相似的分布特征 ,但茨榆坨地区的原油样品的碳同位素值比牛居地区的系统偏轻 ,可能是成熟度相对较低引起的 ,表明茨榆坨地区原油具有早期成藏的特征。原油的碳同位素组成特征是研究油气来源和成藏特征分析的一种重要手段。