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31.
深水重力流作为一种重要的、特殊类型的沉积体系,自发现以来就得到了学术界的广泛关注,并在油气勘探中日益受到重视。东营凹陷古近系沙三中段发育深水重力流体系,综合地震、岩心、测录井等资料,对郝家油田史112区块深水重力流体系的沉积类型、特征及在不同层序中的发育演化进行了精细刻画,总结了该区重力流沉积模式,为开发区储层预测提供重要参考。研究表明,本区深水重力流体系发育于三级层序的高位域,从下至上可划分出4个四级层序(SQQ1-4),主要发育滑塌沉积、碎屑流沉积和浊流沉积3种成因类型,可识别出12种岩相组合。四级层序$\mathrm{SQQ}_{3}^{2}$时期重力流规模较小,$\mathrm{SQQ}_{3}^{3}$时期随着东营三角洲向湖盆中心推进,重力流规模扩大。滑塌沉积主要发育在三角洲前缘或前三角洲斜坡根部,在滑塌沉积前方形成碎屑流沉积,碎屑流向前搬运的过程中,逐渐转化成浊流沉积。三角洲前缘及前三角洲的浊流和碎屑流是开发井区进一步寻找储层的有利部位。 相似文献
32.
通过对陇川盆地开展地热地质调查,查清其地热资源分布:盆地内共出露地热点11处,热储结构类型为带状型和层状型,盆地中部为层状型,两侧盆地边缘为带状型,其中北西部受断裂控制明显,南东部受节理裂隙控制明显。其储热层为变质岩及新近系芒棒组的花岗质砂砾岩、细砂岩;地热水受大气降水影响明显,循环深度都在1 600 m以上,大部分在1 800~2 400 m之间,主要来源于深部热源,通过断裂、裂隙及砂砾石孔隙作为导水、储水上涌通道,接收来自山区补给的地下水混合出露于地表,补给距离在1.5 km以上,如南宛河温泉温度最高,地下水循环深度最深,补给距离最远,达10 km;盆地北东和西部水温高,循环深度深。 相似文献
33.
34.
标准生长曲线(Standardised Growth Curve,SGC)法的提出为高效快速地测定释光样品的等效剂量(De)值提供了可能。不同实验室的放射源剂量率、操作流程、仪器误差等的不同会导致SGC参数的不同。运用最小二乘法标准化实验剂量校正后的信号Lri/Tri*De得到一条本实验室的标准生长曲线,用来快速得到等效剂量值。通过R软件实现了最小二乘法标准化过程,建立了50、100、150、200、250℃激发温度下的钾长石的标准生长曲线,分析发现250℃下的SGC收敛性最好,由于此温度下的信号衰退率可忽略不计,因此,我们用250℃激发温度下的SGC方程来估计样品的等效剂量。比较250℃ SGC De和250℃ MET-pIRIR De的一致性,发现在0~500 Gy范围内用SGC法估计的De和MET-pIRIR法估计的De非常接近,表明了此范围内SGC法的可靠性,而在>600 Gy范围内出现较大差别。一方面,此范围内用于拟合SGC的数据点较少导致高剂量区域内拟合的方程参数不够准确;另一方面,600 Gy与SGC对应的饱和剂量水平值844.5 Gy已经接近,所以在>600 Gy区域测出的De很可能出现较大偏差。因此需在今后工作中逐步积累更多样品,完善SGC参数,使其也能胜任较老年龄样品。 相似文献
35.
Hu Kun Shao Jian-Fu Zhu Qi-Zhi Zhao Lun-yang Wang Wei Wang Ru-Bing 《Acta Geotechnica》2020,15(12):3443-3460
Acta Geotechnica - This study develops a micro-mechanics-based elastoplastic damage model within the framework of irreversible thermodynamics. In the model, damage is related to growth of... 相似文献
36.
Doklady Earth Sciences - Deju basalts is a characteristic volcanic association and was first founded in the 1 : 50 000 regional geological survey. There is no previous... 相似文献
37.
In this work, the elastic buckling of porous solids was investigated using a lattice spring model (LSM). The capability of the LSM to solve elastic buckling problems was comprehensively verified by comparing well-established numerical and analytical solutions. Following this, the buckling of a porous solid was studied, in which two porous structures were considered, ie, the random porous model and the Voronoi porous model. The results reveal that both the porosity and the shape of the pores influence the elastic buckling bearing capacity of the porous solid. Finally, the mechanical responses of a porous solid with an extra high porosity (0.85) were numerically investigated. Our numerical results demonstrated that the nonlinear elastic response of the porous solid might come from its mesoscale elastic buckling. This work shows the ability and promise of using the LSM as a fundamental numerical tool for the deep investigation of the buckling mechanical behavior of porous solids. 相似文献
38.
A local current sheet and a subsequent small interplanetary magnetic-flux rope were observed on 1 April 2003 by Wind and the Advanced Composition Explorer (ACE). A Petschek reconnection-like exhaust crossing of the local current sheet was identified using the Walén test. The Wind spacecraft re-entered the reconnection exhaust after the main exhaust encounter, and the reentry may be due to a spatial fold of the current-sheet surface itself. The absence of parallel strahls and the presence of antiparallel strahls on either side of the current sheet suggest that the magnetic-field lines before the exhaust and in the subsequent small flux rope are all open. The \(180^{\circ}\) pitch-angle strahls were clearly absent, and halo-suprathermal electron pitch-angle distributions were observed in the exhaust. This finding means that the open field lines of the magnetic-flux rope were reconnecting to the adjacent open field lines to produce U-shaped field lines disconnected from the Sun. These observations provide direct evidence that the magnetic fields of the interplanetary small magnetic-flux rope were disconnecting from the Sun through magnetic reconnection. This type of disconnected event potentially has important implications for the magnetic-flux budget of the heliosphere. 相似文献
39.
Ming-Jiang Zhang Hong-Bo Wang Chang-Yin Zhao Jian-Ning Xiong Dong Wei Wei Zhang Sheng-Xian Yu 《Astrophysics and Space Science》2018,363(8):175
Taking the re-entry object CZ-3B R/B (COSPAR identifier 2012-018D, NORAD catalog number 38253) as an example, retrieval of atmospheric mass densities in lower thermosphere below 200 km from its rebuilt precise orbit is studied in this paper. Two methodologies, i.e. analytical and numerical methods, are adopted in the retrieval. Basic principles of these two methodologies are briefly introduced. Based on the short-arc sparse observational data accumulated in the high accuracy re-entry prediction, orbit determinations of re-entry object CZ-3B R/B are performed sectionally, and then its precise orbit is rebuilt. According to the orbit theory, the variation of orbital semi-major axis of re-entry object CZ-3B R/B induced by atmospheric drag perturbation only is derived from the rebuilt precise orbit. In the derivation of secular change of the orbital semi-major axis of re-entry object CZ-3B R/B induced by atmospheric drag perturbation only, the time-span is set as one minute tentatively. And then retrieval results of atmospheric mass densities in lower thermosphere below 200 km by analytical and numerical methods are presented, as well as their bias deviations from the calculated results of the NRLMSISE-00 empirical model of the atmosphere. Setting bias deviation bands, the corresponding ‘confidence coefficients’ of the retrieved atmospheric mass densities with respect to the model values are given. Average bias deviations of the retrieved atmospheric mass densities by analytical and numerical methods from the model values are also calculated respectively. On the whole, the retrieved atmospheric mass densities by numerical method approach to the model values more closely; the differences between the retrieved results and the model values are relatively smaller at the peaks of atmospheric mass densities than the other places. 相似文献
40.
Xuzhen He Dongfang Liang Wei Wu Guoqing Cai Chenggang Zhao Shun Wang 《国际地质力学数值与分析法杂志》2018,42(11):1217-1234
This study uses an incompressible smoothed‐particle hydrodynamics model to investigate the interaction between dry granular material flows and rigid barriers. The primary aim is to summarise some practical guidelines for the design of debris‐resisting barriers. The granular materials are modelled as a rigid‐perfectly plastic material where the plastic flow corresponds to the critical state. The coupled continuity equation and momentum equation are solved by a semi‐implicit algorithm. Compared with flows in controlled flume experiments, the model adequately reproduces both the kinetic of the flows and the impact force under various conditions. Then the numerical simulations are used to study the detailed interaction process. It is illustrated quantitatively that the interaction force consists of two parts, ie, the earth pressure force caused by the weight of the soil and a dynamic force caused by the internal deformation (flowing mass on top of a dead zone). For the estimation of impact load, this study suggests that an increased earth pressure coefficient depending on the Froude number should be incorporated into the hydrostatic model. 相似文献