北冰洋西部表层沉积物矿物学特征及其物质来源

对北冰洋西部79个表层沉积物样品进行了全岩X射线衍射矿物组成分析,结合洋流和地质背景,探讨各矿物分区的物质来源。矿物组合分区表明研究区物质来源变化较为复杂:(1)在楚科奇海的中部靠近白令海峡处长石含量很高,主要是阿纳德尔流携带的来自阿纳德尔河的沉积物;在楚科奇海的西侧的长石含量也较高,且与其他矿物组合分区相比,角闪石含量较高,这是因为受阿纳德尔流和东西伯利亚沿岸流的双重影响,沉积物来自西伯利亚陆地的一些高含长石的火山岩及沉积岩等。在楚科奇海的东侧,石英含量很高,来源为阿拉斯加沿岸流携带的育空河及卡斯奎姆河的沉积物。在阿拉斯加北部,碳酸盐岩和石英含量高,这与马更些河搬运的沉积物有关;(2)北冰洋西部深水区中加拿大海盆的南端和中部方解石和白云石的含量较低,说明受波弗特环流携带的加拿大北极群岛的碳酸盐影响相对较小,且与其他矿物组合分区相比,云母含量最高,说明沉积物主要来源为来自拉普捷夫海的海冰沉积物;此外,一些黏土级细粒物质可能由大西洋中层水携带而来。深水区的其他海域以方解石和白云石含量高为特点,主要受波弗特环流的影响,来源主要为加拿大北极群岛的班克斯岛和维多利亚岛;此外,还受来自西伯利亚陆架,主要是拉普捷夫海沉积物的影响。     

基于ECDIS的多数据源支持技术分析

利用多源地理空间数据集成和融合理论,研究了基于ECDIS的多数据源支持技术。介绍了常用的多源海图数据及其使用原则,分析了ECDIS多数据源支持技术的特点及内涵,总结了国内外常用多源海图数据集成方法,从数据可用性角度探讨了提高国产电子海图系统适用性的措施。     

Mud volcanism and fluid geochemistry in the Cheleken peninsula,western Turkmenistan

A geological and geochemical study has been carried out to investigate the relationships between major mud volcano structures and deep fluid migration in the Cheleken peninsula, in the South Caspian Basin. The fluid geochemistry allowed the origin and migration of the saline waters and the hydrocarbons to be deduced along with the regional source and reservoir rocks. The emitted waters formed by the mixing of deep highly saline water from the main source rocks of the Maykop Fm with the Caspian-like pore water contained in the Pliocene reservoirs. The water composition is very similar to that emitted by the mud volcanoes in Azerbaijan, allowing comparisons to be done between the reservoirs in the western and eastern sides of the South Caspian Basin. The associated oil is derived from a mixed type II/III kerogen deposited in a sub-oxic marine environment and generated during the early oil window. The oil biomarkers indicate that the source rock is the Maykop Fm., as previously determined for the other areas of the South Caspian Basin.The spontaneous emissions, showing different morphologies, are mainly aligned along normal and transtensive fault systems, which provide effective pathways for rapid fluid ascent from deep reservoirs to the surface.     

荣成天鹅湖越冬大天鹅粪便的重金属水平

为对大天鹅(Cygnus cygnus)保护及湖区管理提供基础数据,作者于2011年11月~2012年3月研究了山东荣成天鹅湖越冬大天鹅食物来源及其粪便的重金属水平。结果表明:所选择的食物来源中,Zn、As和Cr在硬毛藻(Chaetomorpha linum)中含量最高,Cd在大叶藻(Zostera marina L.)叶片中含量最高,Pb在大叶藻根茎中含量最高,Cu在石莼(Ulva pertusa)中含量最高,Hg在小麦(Triticum aestivum)中含量最高;水生植物来源的粪便中Cd含量极显著高于陆地植物来源的粪便,陆地植物来源的粪便中Cr,Pb和Hg含量显著高于水生植物来源的粪便;摄食小麦苗可能造成大天鹅对Cd和Hg的积累。     

广西苍梧社垌石英脉型钨钼多金属矿床流体演化及来源示踪

广西苍梧社垌矿床是大瑶山隆起南侧新发现的一个大型斑岩-矽卡岩-石英脉型钨钼多金属矿床。本文重点对其中的石英脉型矿床进行了研究,依据脉体穿插关系及矿物共生组合将成矿过程划分为I石英-黄铁矿阶段、II石英-白钨矿-辉钼矿阶段、III石英-多金属硫化物阶段以及IV石英-方解石-萤石阶段,其中II和III阶段为主成矿阶段。从早到晚,均一温度逐渐下降(第一阶段550℃→370℃,第二阶段370℃→330℃,第三阶段330℃→210℃,第四阶段190℃→150℃),流体密度逐渐上升(0.61g/cm3→0.72g/cm3→0.82g/cm3→0.94g/cm3),盐度先升后降(第一阶段5.86%～8.55%NaCleqv,第二阶段4.49%～43%NaCleqv,第三阶段0.53%～46.37%NaCleqv,第四阶段0%～12.85%NaCleqv)。激光拉曼成分分析显示,社垌石英脉型矿床的成矿流体属于H2O-NaCl体系,但是该体系的流体成分在成矿前后发生了较大的变化,反映第I阶段以氧化环境为主,(II、III、)IV阶段则为还原环境。氢氧同位素研究显示成矿流体来自于岩浆水,后期大气降水的加入导致矿质发生沉淀。此外金属硫化物的δ34S组成(-3.8‰～+1.7‰)平均为-0.46‰,接近于零值,也表明为岩浆来源。引起矿质沉淀的主要原因是流体混合导致的温度下降等环境条件的改变。总体而言,社垌石英脉型钨钼多金属矿床的成矿流体主要来自岩浆热液,为中高温、中低盐度、低密度的NaCl-H2O流体体系,钨钼等多金属成矿与区内加里东期岩浆作用密切相关。     

基于饮水标准的矿山水源人体健康风险--以云南个旧锡矿区某矿坑水源为例

饮水水源水质的人体健康安全是水源是否安全的首要问题。在调查锡矿矿坑水作为个旧市A镇及B矿段锡矿生活区饮用水源情况的基础上,应用国际辐射防护委员会和美国环保署推荐的风险评估模型,开展饮用水的人体健康风险评价。结果表明,水源中重金属致癌物质所引起的健康危害较高,风险值超过了国际辐射防护委员会推荐的最大可接受风险水平,其中以Cr6＋和As的致癌风险最大,应优先控制;非致癌物质所引起的健康风险较小,风险值在10-8以下,远低于推荐的最大可接受风险水平。虽然水中重金属含量符合相关标准要求,但是长期饮用对人体存在健康风险。     

The Converter Mechanism of Particle Acceleration and Its Applications to the Unidentified Egret Sources

We discuss the properties of gamma-ray radiation accompanying the acceleration of cosmic rays via the converter mechanism. The mechanism exploits multiple photon-induced conversions of high-energy particles from charged into neutral state (namely, protons to neutrons and electrons to photons) and back. Because a particle in the neutral state can freely cross the magnetic field lines, this allows to avoid both particle losses downstream and reduction in the energy gain factor, which normally takes place due to highly collimated distribution of accelerated particles. The converter mechanism efficiently operates in relativistic outflows under the conditions typical for Active Galactic Nuclei, Gamma-Ray Bursts, and microquasars, where it outperforms the standard diffusive shock acceleration. The accompanying radiation has a number of distinctive features, such as an increase of the maximum energy of synchrotron photons and peculiar radiation beam-pattern, whose opening angle is much wider at larger photon energies. This provides an opportunity to observe off-axis relativistic jets in GeV–TeV energy range. One of the implications is the possibility to explain high-latitude unidentified EGRET sources as off-axis but otherwise typical relativistic-jet sources, such as blazars.     

Changes to sediment sources following wildfire in a forested upland catchment,southeastern Australia

Few investigations link post‐fire changes to sediment sources and erosion processes with sediment yield response at the catchment scale. This linkage is essential if downstream impacts on sediment transport after fire are to be understood in the context of fire effects across different forest environments. In this study, we quantify changing source contributions to fine sediment (<63 µm) exported from a eucalypt forest catchment (136 ha) burnt by wildfire. The study catchment is one of a pair of research catchments located in the East Kiewa River valley in southeastern Australia that have been the subject of a research program investigating wildfire effects on runoff, erosion, and catchment sediment/nutrient exports. This previous research provided the opportunity to couple insights gained from a range of measurement techniques with the application of fallout radionuclides ¹³⁷Cs and ²¹⁰Pb_ex to trace sediment sources. It was found that hillslope surface erosion dominated exports throughout the 3·5‐year post‐fire measurement period. During this time there was a pronounced decline in the proportional surface contribution from close to 100% in the first six months to 58% in the fourth year after fire. Over the study period, hillslope surface sources accounted for 93% of the fine sediment yield from the burnt catchment. The largest decline in the hillslope contribution occurred between the first and second years after fire, which corresponded with the previously reported large decline in sediment yield, breakdown of water repellency in burnt soils, substantial reduction in hillslope erodibility, and rapid surface vegetation recovery. Coupling the information on sediment sources with hillslope process measurements indicated that only a small proportion of slopes contributed sediment to the catchment outlet, with material derived from near‐channel areas dominating the post‐fire catchment sediment yield response. Copyright © 2011 John Wiley & Sons, Ltd.     

Variations in sediment sources and yields in the Finger Lakes and Catskills regions of New York

The proportional contributions of stream bank and surface sources to fine sediment loads in watersheds in New York State were quantified with uncertainty analysis. Eroding streamside glacial drift, including glaciolacustrine deposits, were examined to help explain variations in the proportional contributions made by bank erosion. Sediment sources were quantified by comparing concentrations of the bomb‐derived radionuclide ¹³⁷Cs in fluvial sediment with sediment from potential source areas such as agricultural soils, forest soils and stream banks. To compare sediment sources in streams containing abundant deposits of fine‐grained glacial drift with watersheds that lacked moderate or extensive streamside deposits, samples were taken from 15 watersheds in the region. The mean contribution of bank erosion to sediment loads in the six streams with glaciolacustrine deposits was 60% (range 46–76%). The proportional contribution of bank erosion was also important in one stream lacking glaciolacustrine deposits (57%) but was less important in the remainder, with contributions ranging from 0 to 46%. Data from this study on the varying contributions of bank erosion and data from past studies of sediment yield in 15 watersheds of New York State suggest that eroding streamside glacial deposits dominate sediment yield in many watersheds. In other watersheds, past impacts to streams, such as channelization, have also resulted in high levels of bank erosion. Copyright © 2007 John Wiley & Sons, Ltd.     

Whipple telescope observations of LS I +61 303: 2004–2006

In this paper we present the results of the past two years observations on the galactic microquasar LS I +61 303 with the Whipple 10 m gamma-ray telescope. The recent MAGIC detection of the source between 200 GeV and 4 TeV suggests that the source is periodic with very high energy (VHE) gamma-ray emission linked to its orbital cycle. The entire 50-hour data set obtained with Whipple from 2004 to 2006 was analyzed with no reliable detection resulting. The upper limits obtained in the 2005–2006 season covered several of the same epochs as the MAGIC Telescope detections, albeit with lower sensitivity. Upper limits are placed on emission during the orbital phases of 0→0.1 and 0.8→1, phases which are not included in the MAGIC data set.