应用核磁共振成像(NMRI)技术研究复合剂驱油特征     

郎东江  王为民  尚根华 《CT理论与应用研究》2006,15(3):11-16

本文应用核磁共振成像技术,在均值、非均值模型中研究了复合剂驱油动态实验过程。观察及分析了复合剂驱油特征和效果,对复合剂驱油段塞前缘进行了实时跟踪,得到了复合剂驱油段塞前缘油墙的形成及剩余油分布与运移的二维图像,给出了复合剂驱油后,剩余油的饱和度分布曲线。实验表明:在层状非均值地层中,若渗透率差异大,复合剂段塞主要进入高渗层,而波及不到低渗层,即复合剂波及效率低。若渗透率差异小,复合剂段塞大部分进入高渗层,有少部分进入低渗层,即复合剂波及效率较高。  相似文献   

http://dx.doi.org/10.1016/j.gsf.2016.09.005   总被引：1，自引：1，他引：0  

Toshikazu Ebisuzaki  Shigenori Maruyama 《地学前缘(英文版)》2017,8(2):275-298

We propose the nuclear geyser model to elucidate an optimal site to bear the first life.Our model overcomes the difficulties that previously proposed models have encountered.Nuclear geyser is a geyser driven by a natural nuclear reactor,which was likely common in the Hadean Earth,because of a much higher abundance of ~(235)U as nuclear fuel.The nuclear geyser supplies the following:(1)high-density ionizing radiation to promote chemical chain reactions that even tar can be used for intermediate material to restart chemical reactions,(2)a system to maintain the circulation of material and energy,which includes cyclic environmental conditions(warm/cool,dry/wet,etc.)to enable to produce complex organic compounds,(3)a lower temperature than 100℃ as not to break down macromolecular organic compounds,(4)a locally reductive environment depending on rock types exposed along the geyser wall,and(5)a container to confine and accumulate volatile chemicals.These five factors are the necessary conditions that the birth place of life must satisfy.Only the nuclear geyser can meet all five,in contrast to the previously proposed birth sites,such as tidal flat,submarine hydrothermal vent,and outer space.The nuclear reactor and associated geyser,which maintain the circulations of material and energy with its surrounding environment,are regarded as the nuclear geyser system that enables numerous kinds of chemical reactions to synthesize complex organic compounds,and where the most primitive metabolism could be generated.  相似文献   

An advanced numerical model of elastomeric seismic isolation bearings   总被引：1，自引：0，他引：1       下载免费PDF全文

Manish Kumar  Andrew S. Whittaker  Michael C. Constantinou 《地震工程与结构动力学》2014,43(13):1955-1974

The nuclear accident at Fukushima Daiichi in March 2011 has led the nuclear community to consider seismic isolation for new large light water and small modular reactors to withstand the effects of beyond design basis loadings, including extreme earthquakes. The United States Nuclear Regulatory Commission is sponsoring a research project that will quantify the response of low damping rubber (LDR) and lead rubber (LR) bearings under loadings associated with extreme earthquakes. Under design basis loadings, the response of an elastomeric bearing is not expected to deviate from well‐established numerical models, and bearings are not expected to experience net tension. However, under extended or beyond design basis shaking, elastomer shear strains may exceed 300% in regions of high seismic hazard, bearings may experience net tension, the compression and tension stiffness will be affected by isolator lateral displacement, and the properties of the lead core in LR bearings will degrade in the short‐term because of substantial energy dissipation. New mathematical models of LDR and LR bearings are presented for the analysis of base isolated structures under design and beyond design basis shaking, explicitly considering both the effects of lateral displacement and cyclic vertical and horizontal loading. These mathematical models extend the available formulations in shear and compression. Phenomenological models are presented to describe the behavior of elastomeric isolation bearings in tension, including the cavitation and post‐cavitation behavior. The elastic mechanical properties make use of the two‐spring model. Strength degradation of LR bearing under cyclic shear loading due to heating of lead core is incorporated. The bilinear area reduction method is used to include variation of critical buckling load capacity with lateral displacement. The numerical models are coded in OpenSees, and the results of numerical analysis are compared with test data. The effect of different parameters on the response is investigated through a series of analyses. Copyright © 2014 John Wiley & Sons, Ltd.  相似文献   

iTRAQ-based proteomic profiling of the marine medaka (Oryzias melastigma) gonad exposed to BDE-47     

C.C. Fong  Y.F. Shi  W.K. Yu  F. Wei  J.P. van de Merwe  Alice K.Y. Chan  R. Ye  Doris W.T. Au  Rudolf S.S. Wu  M.S. Yang 《Marine pollution bulletin》2014

A recent study demonstrated that 2,2′,4,4′-tetrabromodiphenyl ether (BDE-47) may have an adverse effect on the reproduction in marine medaka (Oryzias melastigma), but the molecular mechanisms remain largely unknown. In this study, we investigated the protein expression profiles of male and female gonads of O. melastigma exposed to dietary BDE-47 at two dosages (0.65 and 1.30 μg/g/day, respectively) for 21 days. Extracted proteins were labeled with iTRAQ and analyzed on a MALDI TOF/TOF analyzer, as results, 133 and 144 unique proteins were identified in testis and ovary, respective, and they exerted dose- and sex-dependent expression patterns. In testis, among the 42 differentially expressed proteins; down-regulation of histone variants and parvalbumins implicated BDE-47 may disrupt the spermatogenesis and induce sterility in fishes. In ovary, 38 proteins were differentially expressed; the elevation of vitellogenins and apolipoprotein A–I expression indicated BDE-47 acts as an estrogen-mimicking compound and led to reproductive impairment in O. melastigma.  相似文献   

爆炸、核试验与天然地震的区别（英文）     

Cho  Kwang-Hyun 《应用地球物理》2014,(4):429-436

本文通过地震正演模型和面波振幅数据对比分析了天然地震、爆炸,与核试验数据,以探索改进辨别天然地震与爆炸的方法。所提方法是基于波数域和频率域的双积分变换解。用于研究的地震事件都发生在北朝鲜,其中包括2001年6月26日（39.212°N,125.383°E）和2001年10月30日（38.748°N,125.267°E）所记录的爆炸数据,2006年10月9日（41.275°N,129.095°E）所记录的一次核试验数据、以及2002年4月14日（39.207°N,125.686°E）和2002年6月7日（38.703°N,125.638°E）所记录的两次天然地震。基于这些数据通过地震波分析与理论模拟表明爆炸引起的地震与天然地震有着不同的波型特征。爆炸引起的信号特征是P波的能量较S波强,在爆炸记录上0.05-0.5Hz频率之间Rg波清晰呈现,而在然地震记录上没有。这是由于爆炸地震记录上P波是优势波,与SH成分发生了耦合。  相似文献   

压实黏质砂土脱湿过程影响机制的核磁共振分析     

田慧会  韦昌富  魏厚振  陈盼  程方权 《岩土力学》2014,35(8):2129-2136

通过对具有不同初始含水率和干密度的两种压实黏质砂土的脱湿曲线进行测试、分析和对比,并结合核磁共振技术,探讨了干密度、初始含水率和土样组分对压实黏质砂土脱湿过程的影响规律。利用核磁共振测得了试样在各级吸力下的T2时间（横向弛豫时间）分布曲线,定性地探讨了不同吸力下试样中的水分分布特征,揭示了干密度、初始含水率和土样组分对试样脱湿过程的微观机制影响。试验结果表明：干密度仅在低基质吸力条件下对试样脱湿过程产生重要影响,而在高吸力条件下初始含水率和试样组分起主导作用;核磁共振结果证实在压实黏质砂土中,小孔隙结构主要由初始含水率和试样组分控制,而大孔隙的结构主要取决于干密度;试样组分对压实土的内部结构和孔隙大小分布的影响比初始含水率大。  相似文献   

音频大地电磁法与核磁共振法结合划分含水层的试验     

于向前  赵义平  王明新  刘迪  王文婷  汪馨竹 《吉林大学学报(地球科学版)》2014,44(1):350

为提高应用地球物理方法划分含水层的准确性,提出将音频大地电磁法与核磁共振法结合运用的综合方法。运用该方法在内蒙古巴彦宝力格盆地某区开展野外试验,并将试验结果与该区域供水水文地质详查报告中的水文地质剖面图进行了比对。结果表明：①试验区100 m深度范围内,该方法所揭示的含水层深度、厚度分布与水文地质剖面图基本一致;②据该方法,介质岩性为泥岩、粉质黏土、粉土、气孔状玄武岩和砂砾时,其衰减时间分别为≤30、30～60、60～120、120～260和260～600 ms,据此得到的介质岩性分布与水文地质剖面图高度吻合;③该方法得到的含水层含水量变化与水文地质剖面图的涌水量变化规律一致。因此,运用该方法划分含水层具有很强的可行性,在生产实践中具有推广价值。  相似文献   

FHD分量核旋仪观测系统的抗干扰技术   总被引：1，自引：0，他引：1  

夏忠  稽才建  冯志生  陈兴东  李飞 《地震研究》2005,28(1):102-107

空间电磁波干扰和电源高频谐波干扰是分量核旋仪观测系统的主要干扰源;分量核旋仪观测系统的探头、分量线圈、供电系统及通信线路是主要的干扰途径。作者着重对干扰途径进行了分析,提出了观测系统的抗干扰措施,并分别对探头及信号输入通道、分量线圈、供电系统、通信线路、仪器电路、仪器控制软件进行了全方位的抗干扰设计,新设计提高了分量核旋观测系统的抗干扰能力。  相似文献   

A Study on the Abundance Distribution of Heavy Elements in Metal-poor Stars by the Parameterization Method     

Ge-Ying Xie  Bo ZhangHong-Jie Li  Jin-Jiang HuChen-Pu Li 《Chinese Astronomy and Astrophysics》2011,35(1):29

Based on a large amount of observed data of element abundances in metal-poor stars, taking the abundance distribution of heavy elements in the solar system as a standard, and selecting Sr, Ba and Eu as the typical elements of the three nucleosynthetic processes in metal-poor stars, namely the weak sprocess, main s-process and r-process, we have studied the contributions of the three kinds of neutron-capture processes to the abundance distribution of heavy elements in metal-poor stars, with the parameterization method. It is found that the higher the metal abundance, the greater the contributions of the weak s-process and the chief s-process to the abundances of lighter neutron-capture elements. The heavier neutron-capture elements are mainly produced by the r-process and the chief s-process; and that at low metallicity, the abundances of heavy neutron-capture elements are mainly produced by the r-process. In the early Galaxy, the weak s-process has almost no contribution to the element abundance.  相似文献   

Light‐element abundance variations in globular clusters     

S.L. Martell 《Astronomische Nachrichten》2011,332(5):467-474

Star‐to‐star variations in abundances of the light elements carbon, nitrogen, oxygen, and sodium have been observed in stars of all evolutionary phases in all Galactic globular clusters that have been thoroughly studied. The data available for studying this phenomenon, and the hypotheses as to its origin, have both co‐evolved with observing technology; once high‐resolution spectra were available even for main‐sequence stars in globular clusters, scenarios involving multiple closely spaced stellar generations enriched by feedback from moderate‐ and high‐mass stars began to gain traction in the literature. This paper briefly reviews the observational history of globular cluster abundance inhomogeneities, discusses the presently favored models of their origin, and considers several aspects of this problem that require further study (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献