北京及邻近地区中等以上地震地下流体异常识别与特征研究

系统分析了北京及其邻区多年积累的震例资料, 提出该区的地下流体异常分为趋势上升型中期异常、 转折型中短期异常、 突发型短期异常和短临异常等类型。 运用“同一化”思路、 从属函数、 剩余曲线及原始曲线均方差等异常判定方法, 提取了中等以上地震, 特别是5级以上地震的中、 短、 临异常实例。 通过对流体异常特征的统计分析, 给出了北京及邻近地区的中期、 中短期、 短期和短临异常的时间分布特征, 并对地震前各阶段异常的超前时间进行了总结, 该时间可作为发震时间的预测指标。 在实际应用中可为该区的震情判定提供依据。     

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。     

科尔沁沙地樟子松水分来源贡献率的稳定同位素模型估计(英文)

利用稳定同位素技术测定降水、土壤水、植物茎干水的同位素组成,结合多元线性混合模型(IsoSource)确定科尔沁沙地东南部樟子松人工林内樟子松的根系吸水范围以及各水源的水分贡献率。通过连续观测强降水事件前后樟子松水分来源的变化,探究降水对樟子松水分利用的影响。结果表明樟子松茎干水与20cm以下土层的土壤水同位素组成最为接近,樟子松的水分吸收主要集中在这一层(最大取样深度80cm)。IsoSource模拟结果与观测结果一致,土壤水分条件较好时,大约60%以上的水分来自于20-80cm土层;当这一深度土壤含水量降低时,樟子松将会更多地依赖更深层的土壤水分。樟子松根系分布的最大深度远小于地下水位,因此很难利用到地下水。2009年7月13日14.4mm的降水前后,樟子松茎干水同位素组成的变化表明,降水结束后36小时樟子松可以感应到降水对表层20cm土壤水分的补充,这一土层的水分贡献率在接下来的24小时内迅速降低。不同水分条件下水分来源的多样性表明樟子松能较好地适应沙地生境。     

TROPICAL ATMOSPHERIC NONLINEAR STEADY RESPONSE SOLUTION UNDER EFFECTS OF PAIRED HEAT SOURCES OF CONTRASTING NATURE*

Based on steady semi-geostrophic model equations,analysis is carried out of the linear and nonlinear modification/response of the tropical atmosphere to the forcing of ideal paired heat sources of contrasting nature.Resuits show that the linear part is dominant in the steady response but the nonlinear modification is quite noticable in the neighborhood of the heat source and between the paired sources,and the barotropic mode and second baroclinic mode play a different role in the modification,with the barotropic(second baroclinic)mode modification depending largely on the Rossby wave self-interaction(the magnitude due to the Kelvin-Rossby wave interaction)between the paired sources.     

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.     

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.      

羊石坑汞矿床包裹体地球化学特征研究

羊石坑汞矿是80年代后期勘探的大型汞矿床,矿床位于川黔汞矿带北部,矿体以细脉、网脉浸染状为主。包裹体地球化学研究表明,成矿温度120～250℃,成矿流体盐度为10.6％(NaCl),流体沸腾发生在250℃左右,包裹体圈闭的最小压力为40×10~5Pa,成矿深度约为400m。结合成矿构造环境、构造演化、探讨了构造改造成矿机制和规律。     

C02-CH4流体与金成矿作用：以阿尔泰山南缘和穆龙套金矿为例

造山型金矿的成矿作用与H20-CO2流体有着密切的联系。然而对阿尔泰山南缘和穆龙套金矿的流体包裹体研究表明，无水的CO2-CH4流体在中亚成矿域中一些金矿床中具有同样重要意义。阿尔泰山南缘萨热阔布金矿包裹体的Xch4达0.20～0.23，穆龙套金矿的XCH4为0.07～0.23。CH4扩大了流体不混溶的范围，有利于对Au的富集沉淀。CO2流体在Au成矿中的重要作用至少包括了三方面的意义，即：缓冲流体PH值范围、提高流体中的Au含量并使其维持与还原硫的络合作用进行迁移；扩大超临界流体的温度范围；增加流体不混溶的区域。CH4的加入扩大了流体不混溶的范围，有利于对Au的富集沉淀。     

河南冷水北沟铅锌银矿床流体包裹体研究及矿床成因

河南栾川冷水北沟铅锌银矿床位于华北克拉通南界栾川断裂北侧。矿床赋存于中-晚元古代浅变质碎屑岩建造中,受断裂控制,矿体呈脉状;矿石主要由金属硫化物,少量石英和碳酸盐组成;围岩蚀变和成矿过程分为4个阶段,以石英-黄铁矿组合（Ⅰ阶段）、黄铁矿-闪锌矿组合（Ⅱ阶段）、多金属硫化物（Ⅲ阶段）和碳酸盐（Ⅳ阶段）为标志。包裹体研究表明,成矿流体为含CH4的碳水体系,盐度为0．22～13．8wt％NaCleqv．。从早到晚,流体包裹体均一温度为420℃～340℃（Ⅰ）、3700C～280℃（Ⅱ）、320℃～260℃（Ⅲ）和〈260℃（Ⅳ）。Ⅰ、Ⅱ阶段的流体盐度低于8wt％NaCIeqv．,Ⅲ阶段增高至13．8wt％NaCIeqv．,甚至偶见子晶。Ⅰ、Ⅱ阶段的流体包裹体均一压力分为两组,即180～200MPa和70～80MPa,代表着深约8km的静水与静岩压力系统的共存或交替;Ⅲ阶段只有70～80MPa一组压力,指示开放环境注入的静水压力体系。Ⅰ、Ⅱ阶段静岩与静水压力系统的交替现象完全吻合于断层阀模式,含CH4的CO2-H2O流体的脉动沸腾消耗了流体成矿系统热能,并使盐度不断增高、成矿。该认识可被Ⅱ阶段广泛存在的沸腾流体包裹体组合证明,也与流体包裹体成分类型、矿物共生组合特征、矿石组构的规律演化相一致。以上表明,冷水北沟是一个典型的形成于碰撞造山挤压向伸展转变期的造山型Pb-Zn-Ag矿床实例,成矿机理可由碰撞造山成岩成矿与流体作用模型（即CMF模式）所解释。     

Parameters affecting maximum fluid transport in large aperture fractures

We present results of laboratory experiments to study the behavior of liquids moving in unsaturated wide-aperture fractures. A 5-mm-thick glass plate cut with a 1.7-mm aperture was used as a fractured rock analog to study behavior of film and capillary droplet flow modes. Flow rates ranged between 0.6 and 6.0 ml/min. Variability in the ambient barometric pressure, resulting from weather conditions, seemed to play a role in the natural selection of flow mode. For droplet mode, constant input conditions resulted in highly variable transport properties within the fracture. The advancing meniscus exhibited a dynamic contact angle that was a function of the droplet speed and much larger than the static contact angle. Flow rate was reduced due to the larger contact angle. Analytical expressions for droplet velocity and flow capacity are presented as a function of the dynamic rather than the static contact angle.