南海南部陆缘地质流体类型及其油气成藏意义          下载免费PDF全文

鄢伟  张光学  张莉  夏斌  杨振  雷振宇  林珍  钱星  骆帅兵 《中国地质》2018,45(1):39-47

南海南部陆缘蕴藏着非常丰富的油气资源。为了解南海南部陆缘流体活动系统以及与油气藏之间的关系,以高精度2D地震资料为基础,对南海南部陆缘流体活动系统的类型、地震反射特征、以及对油气成藏的意义开展了研究。在南海南部陆缘发现了多种流体活动系统,包括:泥底辟/泥火山、气烟囱、管状通道、与构造断层相关的流体活动系统。这些流体活动系统具有不同的地震反射特征,常常出现含气强振幅异常带、弱振幅杂乱反射带以及"下拉"或者"上拱"地震反射形态等流体活动系统的标志特征。流体活动系统受到构造运动和沉积因素的影响,并且与深部高温高压塑性流体密切相关,流体活动系统优先发育在地层薄弱部位。流体活动系统及所伴生的断裂和裂隙常常作为油气富集区的运输通道;并且流体活动系统所运移的强溶蚀性流体和深部热液流体有利于油气储层的形成,特别是对于碳酸盐岩储层的改造尤为明显。因此,流体活动系统不仅能作为油气运移通道,也可以改善储层,对油气成藏具有重要意义。  相似文献   

矿用随钻动态方位伽马仪器的研制与应用     

陈龙  陈刚  张冀冠 《煤田地质与勘探》2022,50(1):86-91

顺煤层瓦斯抽采钻孔是目前最直接最有效的瓦斯治理方法,自然伽马作为含煤地层识别常用的判识依据,可以根据地层放射性判断钻孔轨迹是否在目标层中。但现有的矿用伽马测井仪器只能进行滑动钻进测量,不适用于复合钻进及旋转导向钻进,无法满足伽马动态连续测量的工况。针对以上问题,在分析了煤矿井下随钻测量工况特点和伽马测井原理的基础上,通过低压直流载波双向通信技术进行孔底多扇区方位伽马数据的实时传输;采用屏蔽开窗的结构设计,实现单伽马晶体的8扇区分区测量;基于三轴MEMS加速度传感器和三轴MEMS陀螺仪不同的频率特性,采用互补滤波的动态测量方法,克服了回转钻进过程中振动和旋转对工具面向角测量的影响。通过地面性能测试和井下的工业性试验,验证了仪器在不同放射性地层分界面能正确反映出地层放射性变化规律。试验结果表明,仪器可以满足复合回转定向钻进时的地质导向测量要求,为煤矿井下顺煤层定向钻进提供了技术保障。   相似文献   

放射性元素在测井解释中的应用进展及分析     

王敏  李菲 《地质论评》2023,69(Z1):423-424

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高海拔宇宙线观测站LHAASO概况     

曹臻  陈明君  陈松战  胡红波  刘成  刘烨  马玲玲  马欣华  盛祥东  吴含荣  肖刚  姚志国  尹丽巧  查敏  张寿山 《天文学报》2019,60(3):1-16

宇宙线发现百年以来,宇宙线起源仍然是一个谜.研究宇宙线起源主要在甚高能(VHE)伽马射线天文学和宇宙线物理学两个领域交叉展开.新一代高海拔宇宙线观测站(LHAASO)拥有高海拔、全天候和大规模优势,利用多种探测手段对宇宙线开展联合观测,大幅提升对伽马射线和宇宙线的鉴别能力. LHAASO将开展全天区伽马源扫描搜索以大量发现新伽马源,将获得30 TeV以上伽马射线探测的最高灵敏度,将在宽达5个数量级的能量范围内精确测量宇宙线分成份能谱,为揭开宇宙线起源谜团给出重要判据.系统介绍了LHAASO的探测器结构、性能优势和科学目标.  相似文献   

The Review of γ-ray Astronomical Observing Techniques     

《Chinese Astronomy and Astrophysics》2021,45(3):281-300

$\gamma$-ray is a unique probe for extreme events in the universe. Detecting the $\gamma$-ray provides an important opportunity to understand the composition of universe, the evolution of stars, the origin of cosmic rays, etc. $\gamma$-ray astronomy involves in various frontier scientific issues, and the observed energy spectrum spans over a wide range from a few hundreds of keV to a few hundreds of TeV. Different $\gamma$-ray telescopes are in need for different scientific goals and spectral bands. In this work, 5 kinds of space- and ground-based $\gamma$-ray observing techniques were summarized, including the Coded-aperture telescopes, Compton telescopes, Pair-production telescopes, Imaging Atmospheric Cherenkov Telescopes, and Extensive Air Shower Arrays. The progress in $\gamma$-ray astronomy in the past 70 years, motivated by the observation capability, was reviewed. Great achievements have been made in the high-energy domain and very-high-energy domain, while because of the limited missions conducted, as well as a lower sensitivity comparing with other domains, discoveries in low- and medium-energy are few, and due to the high observation difficulty, as well as the late start, relevant scientific yields in ultra- and extremely-high energy are limited. Moreover, the future planned missions and capabilities of the $\gamma$-ray telescopes and their possible scientific outputs were discussed. Among these missions, low- and medium-energy space telescopes e-ASTROGAM (enhanced-ASTROGAM), AMEGO (All-sky Medium Energy Gamma-ray Observatory), and very-high-energy ground-based arrays LHAASO (Large High Altitude Air Shower Observatory) and CTA (Cherenkov Telescope Array) greatly improve sensitivity than their corresponding last generation, thus expect very likely to further expand our knowledge on the $\gamma$-universe.  相似文献   

Reservoir architecture and heterogeneity distribution in floodplain sandstones: Key features in outcrop,core and wireline logs     

Luis Miguel Yeste  Augusto N. Varela  César Viseras  Neil D. Mcdougall  Fernando García-García 《Sedimentology》2020,67(7):3355-3388

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Data Analysis of Chang’E-1 Gamma-Ray Spectrometer and Global Distribution of U, K, and Th Elemental Abundances     

ZOU Yongliao  ZHANG Liyan  LIU Jianzhong  MU Lingli  REN Xin  ZHANG Guangliang  CHANG Jin  YAN Jun  ZHANG Nan  ZHANG Hongbo  Lü Chang  LIU Jianjun  ZUO Wei  SU Yan  WEN Weibin  BIAN Wei  WANG Min  XU Chun  LI Chunlai  OUYANG Ziyuan 《《地质学报》英文版》2011,85(6):1299-1309

Gamma-ray spectrometer (GRS) is one of the main payloads on the Chang’E-1 (CE-1) lunar probe, mainly aimed to detect the elemental abundances and distributions on the lunar surface. At 03:58 on 28 November 2007, it performed the first observation of the lunar gamma rays. As of 24 October 2008, 2105?h of effective gamma rays spectra had been acquired by CE-1 GRS, which covers the whole surface of the moon. This paper mainly describes the data processing procedures and methods of deriving the elemental abundances by using the CE-1 GRS time series corrected spectra: first, to bin data into pixels for mapping; then, to perform a background deduction of the cumulative spectra and obtain a peak area of the elements; and finally, to use the elemental abundances inversion model to produce the elemental abundances. Based on these processing methods, the global abundance maps of U, K, and Th at a 5°×5° equal-area pixel are acquired by CE-1 GRS data. The paper gives a preliminary analysis of the uncertainties of the elemental abundances  相似文献   

张掖市平山湖地区煤岩层物性规律研究与测井方法应用     

张元基 《中国煤炭地质》2011,(6):59-64

通过对平山湖地区11口井的测井资料进行分析,初步掌握了该区含煤岩层的地球物理特性及其在视电阻率、密度、自然伽马、声波时差、自然电位等测井曲线上的响应特征。总结出一套适合该地区的测井方法,如各种测井参数的数据计算方法与曲线处理技巧,为该类地区使用TYSC-3Q测井仪器进行测井提供了参考依据。针对该地区煤层具有中高阻、低密度、低放射性、高时差、弱自然电位的物性特征,以多个实例介绍了煤层在不同测井参数曲线上的识别方法及定量解释原则。  相似文献   

雨滴谱的变化对降水估计的影响     

吴亚昊  周筠珺  刘黎平 《成都信息工程学院学报》2015,30(2)

针对雨滴谱的变化对降水估计的影响,提出根据激光雨滴谱仪上方雷达回波的结构特征将降水过程划分为对流云降水和层状云降水交替分布5个部分,通过基于2种降水类型的第1种分类Z-R关系、基于5个部分的第Ⅱ种分类Z-R关系和基于整个降水过程的总体Z-R关系分析雨滴谱的变化对降水估计的影响.结果表明:当对流云降水向层状云降水过渡时,指数谱从无到有、多峰谱比例减小,Nw减小、μ增大、Dm变化不大;Mw与R变化相似,当Z增大时μ和Dm分别是递减和递增的;Z-R关系(Z=aRb)中a值变化范围较大、系数b在1～2波动且与层状云阶段相比,对流云阶段的a和b值较小;利用第Ⅱ种分类Z-R关系反演的雨强与基于雨滴谱仪观测数据计算的雨强最接近;雨滴谱仪在层状云阶段的反演效果明显强于对流云阶段,这与对流云降水中雨滴谱信息变化大且快等因素有关.  相似文献   

综合物化探方法在深冲矿区铀多金属矿勘探中的应用     

何友宇  覃金宁  李竹溢  黄绍琼 《国土资源导刊(湖南)》2015,(1):84-89

通过研究深冲铀矿区γ能谱铀异常、氡浓度异常特征和激电异常特征,探索矿区范围岩体、断裂构造和蚀变带与物化探信息显示特征的关系。据此,结合矿区地质特征,总结物化探方法应用效果,矿致异常综合特征。  相似文献