四川盆地广安地区中二叠统栖霞组岩石特征与沉积环境     

易海永  崔宝琛  王瑶琳  邱玉超  徐胜林  李乾 《吉林大学学报(地球科学版)》2020,50(2):454-464

四川盆地中二叠统栖霞组勘探发现系列油气，资源潜力巨大。但广安地区中二叠统栖霞组的岩石学特征及沉积环境研究薄弱。在野外地质调查的基础上，结合室内岩石学、岩相学等综合分析，对广安地区栖霞组碳酸盐岩岩石特征、沉积相类型及其古地理展布特征进行了系统研究。结果表明：广安地区栖霞组主要发育亮晶颗粒灰岩、亮晶生物碎屑灰岩、微晶生物碎屑灰岩、微晶颗粒灰岩、生物碎屑微晶灰岩、含生物碎屑微晶灰岩和泥晶灰岩7种岩石类型；碳酸盐岩颗粒主要以生物碎屑为主，部分层位发育球粒；古生物化石以三叶虫、腕足和有孔虫为主，同时可见棘皮类和藻类；栖霞组沉积期主要为碳酸盐岩台地沉积环境，其中栖霞组晚期（栖二段）台缘滩和台内滩较为发育，为该区油气成藏提供了有利条件。  相似文献   

基于振动台试验的移动通信节点机房蓄电池组地震易损性分析          下载免费PDF全文

毛晨曦  冯利飞 《世界地震工程》2019,35(3):010-20

关键移动通信设备的地震易损性是城市移动通信系统地震灾害预测的基础。本文以移动通信系统节点机房中常用的蓄电池组作为研究对象，通过振动台试验来研究蓄电池组的抗震性能，并获得其地震易损性。试验过程中，首先采用FEMA P695建议的方法从美国PEER强震数据库中遴选出对蓄电池组较为危险的地震动记录作为试验激励，随后逐步增大各条地震动记录的幅值，基于振动台进行增量动力分析。试验后根据蓄电池组的地震损伤特征，定义了其损伤指标和损伤水平，并基于振动台试验数据分析获得了典型蓄电池组的地震易损性曲线。  相似文献   

Study of subsurface eddy properties in northwestern Pacific Ocean based on an eddy-resolving OGCM     

Xu  Anqi  Yu  Fei  Nan  Feng 《Ocean Dynamics》2019,69(4):463-474

Ocean Dynamics - A method based on the Okubo–Weiss parameter was used to detect subsurface eddies (SSEs) with an eddy-resolving ocean general circulation model. Statistical analyses showed...  相似文献   

基于区域水准和跨断层资料分析云南地区地壳形变     

徐东卓  苏广利  王世进  朱传宝  孙非非 《震灾防御技术》2019,14(1):118-128

为了获取云南地区现今地壳形变和断层活动特征，收集了云南地区1992—2016年的2期精密水准观测资料，采用基于GNSS连续站垂直形变资料约束的平差方法，对区域整体地壳垂直形变特征进行了分析，结果显示滇西北区域地壳整体表现为隆升，垂向速率为2—3mm/a，滇南区域显示地壳沉降速率为-1—-2mm/a，并在下关—永胜和思茅—景谷一带存在地壳形变高梯度带。收集了该地区30多年的跨断层场地观测资料，计算了所跨断层的三维活动量，得出了断层现今活动状态和异常特征，认为滇西北和滇中南地区的场地多数表现出异常活动的现象，其中楚雄、剑川和永胜的监测断层现今表现出与地质背景相反的走滑和拉张特征，峨山、建水和通海场地所处断层在张压性质上与地质背景相反。结合区域水准和跨断层观测分析结果，从“面”和“线”上得出滇西北和滇中南地区存在地壳形变和断层活动异常，构造应力积累较高的结果，加之缺震背景显著，认为应关注该区域中强地震的危险性。  相似文献   

尼泊尔M_S 8.1地震与青藏高原周边地区多尺度重力场特性分析     

闫琳琳  吕传振  徐玉健 《震灾防御技术》2019,14(1):129-137

通过分析EGM2008模型提取的青藏高原及周边地区重力场细节信息，概述了尼泊尔M_S 8.1地震的均衡重力异常特征，并结合GPS数据对研究区的动力学进行综合分析。结果表明，在喜马拉雅山脉地震带区存在重力的正、负值异常区及梯度带，这与该研究区局部应力应变积累、构造活动加剧、深部物质向研究区迁移以及研究区局部密度增高有关。  相似文献   

偏振激光雷达探测大气—水体光学参数廓线   总被引：2，自引：2，他引：0  

周雨迪  刘东  徐沛拓  毛志华  陈鹏  刘志鹏  刘群  唐培钧  张与鹏  王雪霁  任佳炜  金时伟 《遥感学报》2019,23(1):108-115

激光雷达在上层水体垂直廓线的遥感中展现出巨大优势。本文研制了一套高垂直分辨率的实时探测偏振激光雷达,提出了一种基于偏振激光雷达回波信号的反演算法,采用Fernald理论和多次散射原理反演非均匀大气—水体的衰减和退偏光学产品,以高效稳定地处理偏振激光雷达实验数据。展示了一个中国内陆水体激光雷达探测实例,观测到了两次气溶胶积聚现象和一次水体浑浊现象。对实验数据的分析表明,退偏比主要由前向多次散射和后向单次散射产生的退偏两部分组成。当多次散射强度较大时,退偏比的变化主要取决于多次前向散射退偏;反之,则主要依赖于单次后向散射退偏。  相似文献   

考虑填充墙影响的钢筋混凝土厂房结构地震易损性分析     

梁志强  徐超  温增平 《震灾防御技术》2019,14(4):707-718

采用对角斜撑模拟纵向填充墙的作用，建立考虑填充墙和不考虑填充墙厂房结构模型，采用拉丁超立方抽样技术建立考虑材料不确定性的结构分析样本，基于随机Pushover分析确定结构不同破坏状态下的统计参数。综合考虑结构材料强度及输入地震动不确定性的影响，通过非线性时程分析开展单层钢筋混凝土厂房结构易损性研究，在此基础上比较结构横、纵向易损性的差异，研究填充墙对结构易损性的影响。研究结果表明:钢筋混凝土厂房结构体系横向地震易损性显著大于纵向地震易损性；对纵向结构体系而言，加入填充墙会明显降低结构易损性，但在相同强度的地震动作用下，填充墙破坏程度比主体结构严重，这与厂房结构的实际震害特征相符。  相似文献   

Research on the Application of Fast-steering Mirror in Stellar Interferometers     

Mei Rong  Hu Zhong-wen  Xu Teng  Sun Chang-sheng 《Chinese Astronomy and Astrophysics》2018,42(3):475-486

In stellar interferometers, the fast-steering mirror (FSM) is widely utilized to correct the wavefront tilt caused by the atmospheric turbulence and internal instrumental vibration, because of its high resolution and fast response frequency. In this study, the non-coplanar error between the FSM and the actuator deflection axis introduced by the manufacturing, assembly, and adjustment is analyzed systematically. Via a numerical method, the additional optical path difference (OPD) caused by the above factors is studied, and its effect on the fringe tracking accuracy of a stellar interferometer is also discussed. On the other hand, the starlight parallelism between the beams of two arms is one of the main factors for the loss of fringe visibility. By analyzing the influence of wavefront tilt caused by the atmospheric turbulence on fringe visibility, a simple and efficient real-time correction scheme of starlight parallelism is proposed based on a single array detector. The feasibility of this scheme is demonstrated by a laboratory experiment. The results show that after the correction of fast-steering mirror, the starlight parallelism meets preliminarily the requirement of a stellar interferometer on the wavefront tilt.  相似文献   

Petrogenesis of Early Cretaceous hornblende gabbro in Khanka Massif: evidence from geochronology and geochemistry     

WEI Chunxia  WEI Xu  ZHU Weigang  XU Wenliang 《世界地质(英文版)》2018,(3)

The authors report zircon U-Pb geochronological,whole-rock geochemical and zircon Lu-Hf isotope data for the hornblende gabbro within the Khanka Massif,with the aim of constraining its formation time and petrogenesis. The zircon U-Pb dating shows that ~(206)Pb/~(238)Pb ages of zircons from the hornblende gabbro range from 120 to 129 Ma,yielding a weighted mean age of 123 ± 2 Ma,i. e.,the Early Cretaceous. The hornblende gabbro has SiO_2 of 44. 77%--46. 58% and belongs to the tholeiitic series on FeO~t/MgO-SiO_2 diagram. It displays a right-inclined REE pattern with( La/Yb)_N ratios of 3. 44 to 4. 42. The trace element spidergram shows that they are enriched in large ion lithophile elements( LILE) such as Rb,Th,U,K and Pb,and depleted in high field strength elements( HFSE) such as Nb,Ta,Ti and P,indicating an affinity to arc igneous rocks.The ε_(Hf)( t) values of zircons vary from -2. 6 to + 3. 9 and Hf model ages( T_(DM1)) range from 622 to 883 Ma.These geochemical characteristics indicate that primary magma of the hornblende gabbro could be derived from partial melting of young mantle material accreted during the Neoproterozoic. Combined with the Early Cretaceous igneous rock assemblages in NE Asia. It is concluded that the hornblende gabbro formed in an active continental margin related to the westward subduction of the Paleo-Pacific Plate beneath the Khanka Massif.  相似文献   

An algorithm to resolve γ-rays from charged cosmic rays with DAMPE     

Zun-Lei Xu  Kai-Kai Duan  Zhao-Qiang Shen  Shi-Jun Lei  Tie-Kuang Dong  Fabio Gargano  Simone Garrappa  Dong-Ya Guo  Wei Jiang  Xiang Li  Yun-Feng Liang  Mario Nicola Mazziotta  Maria Fernanda Munoz Salinas  Meng Su  Valerio Vagelli  Qiang Yuan  Chuan Yue  Jing-Jing Zang  Ya-Peng Zhang  Yun-Long Zhang  Stephan Zimmer 《天文和天体物理学研究(英文版)》2018,(3)

The DArk Matter Particle Explorer(DAMPE),also known as Wukong in China,which was launched on 2015 December 17,is a new high energy cosmic ray and γ-ray satellite-borne observatory.One of the main scientific goals of DAMPE is to observe Ge V-Te V high energy γ-rays with accurate energy,angular and time resolution,to indirectly search for dark matter particles and for the study of high energy astrophysics. Due to the comparatively higher fluxes of charged cosmic rays with respect to γ-rays,it is challenging to identify γ-rays with sufficiently high efficiency,minimizing the amount of charged cosmic ray contamination. In this work we present a method to identify γ-rays in DAMPE data based on Monte Carlo simulations,using the powerful electromagnetic/hadronic shower discrimination provided by the calorimeter and the veto detection of charged particles provided by the plastic scintillation detector. Monte Carlo simulations show that after this selection the number of electrons and protons that contaminate the selected γ-ray events at～10 Ge V amounts to less than 1% of the selected sample.Finally,we use flight data to verify the effectiveness of the method by highlighting known γ-ray sources in the sky and by reconstructing preliminary light curves of the Geminga pulsar.  相似文献