西沙群岛西琛一井礁序列成岩作用研究

西琛一井０－４００米段是西沙礁序列研究内容最丰富，实验分析最多的全取芯钻 ，通过薄征观察，电子探针分析，不同井深单一属腹足类壳体，同一深度不同沉积物的碳 ，氧稳定同位素测定和Ｍｇ／Ｃａ，Ｍｇ／Ｓｒ分析，对西琛一礁序成岩体环境，作用性质及其特征，进行了全面系统的论述，并提出了泥晶套的非藻类穿忆和白云石化的非混合水成因素。     

基于MODIS数据的2016年黄海绿潮灾害动态监测研究

本研究利用高分辨率的GF-1卫星影像对MODIS数据绿潮监测的精度进行验证, 并在此基础上利用MODIS数据对2016年黄海绿潮过程进行连续动态监测, 结果表明: 相较于GF-1卫星影像,MODIS数据对绿潮的监测误差高于50%; 2016年黄海绿潮移动路径总体呈先向北, 然后沿山东半岛海岸线向东北方向移动, 并最终停滞于青岛、威海附近海域; 此次绿潮持续时间为80天左右, 并呈现出与往年类似的“出现→发展→暴发→治理→消亡”的规律; 其中“出现”的时间为5月12日, “发展”阶段时间为5月中下旬, 此时绿潮主体分布于苏北浑水区, 适宜前置打捞治理, 当5月底6月初绿潮进入清水区之后才开始进入“暴发”阶段, 本年度绿潮灾害“暴发”规模较大, 对山东沿海水产养殖业及旅游业影响严重。本研究成果对于绿潮预警和防控具有科学和实际意义。     

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山东东辛油田古近系沙河街组一段碳酸盐岩储集特征

山东东辛油田古近系沙河街组一段湖相碳酸盐岩过去仅作为盖层而忽视其油气地质意义。研究表明,其岩性以生物灰岩及鲕粒灰岩为主,并有少量螺灰岩。其中生物灰岩中以溶蚀孔隙、生物体腔孔及骨架孔隙等类型构成主要的油气储集空间,使其具有较高的孔渗性;鲕粒灰岩在形态上以长条鲕、圈层鲕最为常见,其核心以生物碎片（化石）为主,鲕粒灰岩以粒间孔和粒内孔作为主要的油气储集空间,亦具有较高的孔渗性。沙一段碳酸盐岩的主要矿物成分为白云石和方解石,且大部分白云石及部分方解石均含铁,不同岩性的储层具有不同的储集类型,储层性质受岩石类型、沉积环境、表生作用及胶结作用、溶解作用及白云岩化等成岩作用影响,且沙一段储层处于油气运聚非常有利的过渡带,在藻滩及高能浅滩部位可形成较好的油气富集带,所以对湖相碳酸盐岩储层的研究有助于老区滚动勘探开发。     

火星轨道器次表层探测雷达的水冰探测

在地球上,水是生命存在的基础之一.大量证据表明火星表面曾经存在液态水,而目前的火星表面环境不支持液态水的长期存在.因此,水可能以不同的状态赋存于火星的次表层.寻找火星次表层的水一直是火星探测的关键科学目标之一.次表层探测雷达,如探地雷达、探冰雷达,是了解地下物质结构的有效方法,近年来在地外天体上得到大量应用.在过去十余...     

510—1铀矿床构造、地球化学特征及其成因探讨

本文根据510—1铀矿床形成的构造条件和地球化学特征,认为该富铀矿床的成因是地洼阶段壳幔混合型深源热液上升侵位,与贡巴—益哇逆冲推覆构造上盘中、下志留统羊肠沟组硅灰岩含水含矿层屏蔽构造相结合的结果。并指出古今统一的四维空间屏蔽构造是找矿的方向。     

元页HF-1页岩气水平井钻井关键技术

元页HF-1井是中石化部署在川东北元坝区块的第一口页岩气预探水平井。通过分析该井的工程地质难点,优化了三开次井身结构,优选出合理的钻井方式、钻井液体系和配套工艺措施,形成了一套适合该区块的页岩气水平井钻井技术方案。该井成功钻达目的层,完钻井深4982 m,水平位移1421.73 m,钻井周期168.88 d,平均机械钻速3.07 m/h,三开井径扩大率仅为4.82%,取得良好的应用效果,为元坝区块页岩气的勘探开发提供了技术支撑。     

Integrated methodology for determining provenance of detrital quartz using optical petrographic microscopy and cathodoluminescence (CL) properties

The provenance of detrital quartz is a useful predictor in frontier basin sandstone reservoirs of the availability of coarse-grained quartz grains of plutonic or high grade metamorphic origin. The standard approach is to use scanning electron microscope (SEM) panchromatic cathodoluminescence (CL) imagery and observations from an optical petrographic microscope. We describe a work flow, modified from previous literature proposals, to determine quartz provenance in detrital grains using optical petrographic microscopy and CL properties from both a hot-cathode cathodoluminescence microscope attachment (HCMA) and panchromatic SEM-CL. HCMA analysis permits better discrimination of different types of metamorphic quartz. This method is applied to a Middle Jurassic to Lower Cretaceous section in the Bandol-1 wildcat well, located in the Laurentian sub-basin south of Newfoundland. Two types of high-grade metamorphic quartz are distinguished, one with low luminescence as described in previous literature and one with medium blue CL colour and a moderate colour shift that is also known from granulite in the hinterland. Three phases of detrital supply are identified, suggesting progressive unroofing of higher grade metamorphic sources through the middle Jurassic and major input of plutonic quartz in the early Cretaceous.     

Search for radio pulsations in four anomalous X-ray pulsars and discovery of two new pulsars

We have performed deep searches for radio pulsations from four southern anomalous X-ray pulsars (AXPs) to investigate their physical nature in comparison with the rotation powered pulsars. The data were acquired using the Parkes radio telescope with the 1.4 GHz multibeam receiver. No pulsed emission with periodicity matching the X-ray ephemeris have been found in the observed targets down to a limit of ∼0.1 mJy. A blind search has also been performed on all the 13 beams of the multibeam receiver (the central beam being pointed on the target AXP), leading to the serendipitous discovery of two new radio pulsars and to the further detection of 18 pulsars. Also a search for single dispersed pulses has been performed in the aim to detect signals similar to those of the recently discovered rotating radio transients.      

HESS observations of extragalactic objects

The HESS experiment (High Energy Stereoscopic System), consisting of four imaging atmospheric Cherenkov telescopes (IACTs) in Namibia, has observed many extragalactic objects in the search for very high energy (VHE) γ-ray emission. These objects include active galactic nuclei (AGN), notably Blazars, Seyferts, radio galaxies, starburst galaxies and others. Beyond the established sources, γ-ray emission has been detected for the first time from several of these objects by HESS, and their energy spectra and variability characteristics have been measured. Multi-wavelength campaigns, including X-ray satellites, radio telescopes, and optical observations, have been carried out for AGNs, in particular for PKS 2155-304, H 2356-309 and 1ES 1101-232, for which the implications concerning emission models are presented. Also results from the investigations of VHE flux variability from the giant radio galaxy M 87 are shown. For the HESS Collaboration.