中国资源外交的地缘政治分析

资源外交寓于国际地缘政治的长期博弈之中。地缘政治是一国对外交往所要考虑的重要因素之一。本文立足于内线周边和外线外围的地缘关系分析,总结了中国资源外交地缘政治的总体态势和潜在风险,并试图提出我国资源外交的基本思路。在全球地缘政治格局中,中国的资源外交包括内线地带和外线地带两个层次：内线由接壤的邻国以及接近的近邻组成,是中国资源外交的战略依托地带;外线由涵盖美洲、欧洲、非洲和澳洲大陆的资源生产大国和消费大国组成,是中国资源外交的战略腾挪空间。在这两个层次上,我国的地缘风险主要来自其他大国的地缘战略遏制、“走出去”战略的地缘选择权旁落、资源通道和贸易路线受制于人。要突破这些地缘限制与束缚,我国的资源外交需统筹国内、国际两个大局,分清内线、外线战略方向的轻重缓急,以周边关系为首要、以大国关系为关键、以发展中国家关系为基础,积极拓展对外友好关系的发展空间,有序扩展资源合作领域,坚定维护国家资源权益。     

On the hydraulic intake shape factor for a circular opening located at an impervious boundary: Influence of inclined stratification

In this paper, we develop an exact closed form solution for a circular entry point located at the interface between an impermeable material and a stratified porous medium, where the principal plane of hydraulic isotropy is inclined to the interface. Copyright © 2010 John Wiley & Sons, Ltd.     

Hubble Space Telescope imaging of the progenitor sites of six nearby core-collapse supernovae

The search for the progenitors of six core-collapse supernovae (CCSNe) in archival Hubble Space Telescope ( HST ) WFPC2 pre-explosion imaging is presented. These SNe are 1999an, 1999br, 1999ev, 2000ds, 2000ew and 2001B. Post-explosion imaging of the SNe, with the HST ACS/WFC, has been utilized with the technique of differential astrometry to identify the progenitor locations on the pre-explosion imaging. SNe 1999br, 1999ev, 2000ew and 2001B are recovered in late-time imaging, and estimates of the progenitor locations on the pre-explosion imaging, with subpixel accuracy, have been made. Only the progenitor of the Type II-P SN 1999ev has been recovered, on pre-explosion F555W imaging, at a 4.8σ significance level. Assuming a red supergiant progenitor, the pre-explosion observation is consistent with   M _ZAMS= 15–18 M_⊙  . The progenitors of the other five SNe were below the 3σ detection threshold of the pre-explosion observations. The detection thresholds were translated to mass limits for the progenitors by comparison with stellar evolution models. Pre-explosion observations of the peculiarly faint SN 1999br limit the mass of a red supergiant progenitor to   M _ZAMS < 12 M_⊙  . Analysis has been extended, from previous studies, to include possible detections of high- T _eff, high-mass stars by conducting synthetic photometry of model Wolf–Rayet star spectra. The mass limits for the Type II-P SNe 1999an and 1999br are consistent with previously determined mass limits for this type of SN. The detection limits for the progenitors of the Type Ibc SNe (2000ds, 2000ew and 2001B) do not permit differentiation between high-mass Wolf–Rayet progenitors or low-mass progenitors in binaries.     

Influence of underground space development mode on the groundwater flow field in Xiong’an new area

The degree and scale of underground space development are growing with the continuous advancement of urbanization in China. The lack of research on the change of the groundwater flow field before and after the development of underground space has led to various problems in the process of underground space development and operation. This paper took the key development zone of the Xiong’an New Area as the study area, and used the Groundwater modeling system software (GMS) to analyse the influence on the groundwater flow field under the point, line, and surface development modes. The main results showed that the underground space development would lead to the expansion and deepening of the cone of depression in the aquifer. The groundwater level on the upstream face of the underground structure would rise, while the water level on the downstream face would drop. The “line” concurrent development has the least impact on the groundwater flow field, and the maximum rise of water level on the upstream side of the underground structure is expected to be approximately 3.05 m. The “surface” development has the greatest impact on the groundwater flow field, and the maximum rise of water level is expected to be 7.17 m.     

鄂尔多斯盆地延长探区低渗致密油气成藏理论进展及勘探实践

延长石油集团在鄂尔多斯盆地大力推动石油、天然气、页岩气勘探开发理论研究和技术攻关,多类型资源协同发展,取得显著效果。在石油勘探方面,提出延长组特低渗石油“交替式”成藏理论认识,建立盆地中生界多期差异性成藏新模式,近10年特低渗石油年均探明地质储量超1×10⁸ t。建立细粒沉积风暴、地震等控砂理论,以及甜点预测方法,致密油累计探明地质储量2.1×10⁸ t。针对致密气田砂体成因机理不明、天然气运聚成藏规律不清等主要难题,揭示了“浅水环境岸线频繁迁移控砂”机制,建立了致密砂岩气优质储层成储模式,明确纯石英砂岩和富石英低塑性颗粒岩屑砂岩是致密气分布的“甜点”,形成了基于多要素、全过程天然气运聚模拟的目标优选技术。经勘探实践,发现了延安气田,累计探明天然气地质储量7 635×10⁸ m³。页岩气方面,提出陆相页岩气“三元”成藏富集地质理论的创新认识,认为湖相优质页岩是陆相页岩气富集高产的物质基础,多类型、跨尺度的复杂孔隙网络决定页岩气赋存条件,厚层页岩自封闭能力及高压是保存的关键,实现陆相页岩气产量突破。未...     

大兴安岭地区古生代构造格架重建:来自俯冲增生杂岩研究进展

大兴安岭地区古生代处于古亚洲洋闭合阶段,其间发育众多的弧盆系和蛇绿岩带,笔者等在大兴安岭地区1: 1 000 000地质编图和野外地质调研基础上,应用“洋板块地质”学术思想在大兴安岭地区元古宙、古生代地质体中划分出一系列“俯冲增生杂岩”、地块基底残块、岛弧、弧前盆地、弧后盆地等构造单元,结合陆(地)块和岩浆弧、弧前盆地、弧后盆地和“俯冲增生杂岩”的时空展布,划分出9条俯冲增生杂岩带,其中新识别出3条俯冲增生杂岩带。俯冲增生杂岩带主要分布于兴蒙造山带内部各地块之间和地块与大型岛弧带之间,相当于地块间及地块与岛弧带间的缝合带。依据俯冲增生杂岩带两侧对应的陆(地)块、岛弧带等构造级别,归并出5条结合带。俯冲增生杂岩带的展布方向以北东向为主,时代自北向南依次变新,从早奥陶世演化到中—晚二叠世,暗示古亚洲洋洋盆向大兴安岭地区陆(地)块俯冲作用最早发生在北部额尔古纳一带,逐渐向南后撤,不断形成新的洋壳和产生俯冲增生作用,相应的活动陆缘从北部额尔古纳地块向南逐渐增生,配套弧盆系时代也逐渐向南变新。早—中三叠世至西拉木伦一带发生陆-陆拼贴,完成华北板块与西伯利亚板块的对接。通过对大兴安岭地区古生代“俯冲增生杂岩”的研究,重建了大兴安岭地区古生代构造格架,提高了古亚洲洋东段洋-陆转换的研究程度。     

大兴安岭中生代火山岩地层时空分布与蒙古—鄂霍茨克洋、古太平洋板块俯冲作用响应

为了提高大兴安岭中生代火山岩地层的区域可对比性、深入研究大兴安岭中生代火山岩与古太平洋和蒙古—鄂霍茨克洋的构造关系,本文在大兴安岭地区1: 1 000 000地质图编图的基础上,依据岩石组合、古生物、接触关系、区域对比以及最新的年代学(锆石U-Pb、⁴⁰Ar/³⁹Ar测年)资料,对大兴安岭中生代火山岩地层重新进行了厘定。进一步界定了塔木兰沟组(172~161 Ma)、满克头鄂博组(162~148 Ma)、玛尼吐组(158~145 Ma)、白音高老组(145~129 Ma)、梅勒图组(143~128 Ma)、龙江组(128~120 Ma)、光华组(128~118 Ma)、甘河组(120~113 Ma)和孤山镇组(118~110 Ma)的形成时代。结合古太平洋、蒙古—鄂霍茨克洋板块对东亚大陆边缘的俯冲作用,解析了中生代火山岩形成的构造背景,认为中—晚侏罗世NE向展布的火山岩主要形成于蒙古—鄂霍茨克洋板块向南东俯冲的伸展背景,早白垩世NNE向展布的火山岩主要形成于伊泽奈岐板块向东亚大陆俯冲的伸展背景。晚侏罗世与早白垩世火山岩地层之间发育的开库康组、木瑞组等类磨拉石建造,是两个构造体系转换阶段的主要沉积记录。     

雄安新区D01井岩溶热储下伏太古界中热流测定研究

【研究目的】目前雄安新区范围内的热流数据多测自于新近系沉积盖层及白云岩地层,对岩溶热储下伏太古界的热流测定研究还鲜见报道,主要受限于以往的地热勘查开发层位主要在1800m以浅的蓟县系岩溶热储,揭露岩溶热储下伏太古界的钻孔稀少。2018年以来,在雄安新区牛驼镇地热田实施了D01深部地热参数井,揭穿了高于庄组岩溶热储,并揭露太古界厚度达1723.67m,给该地区岩溶热储下伏太古界的热流测定研究提供了条件。【研究方法】本文基于近稳态钻孔测温及岩心热导率测试,对D01井太古界进行了热流测定及分析。【研究结果】结果表明：D01井太古界呈显著的传导型地温特征,地温梯度为18.3℃/km,相比于新近系地温梯度48.6℃/km偏低。测得25块D01井太古界片麻岩岩心样品的热导率平均值为（2.41±0.40）W/(K·m)。根据钻孔测温数据及热导率测试,计算出D01井太古界2300～2700m深度的热流值为（44.1±7.0）mW/m²。同时,估算了D01井新近系400～800m深度段的热流值为84.6mW/m²,较太古界高出40.5mW/m²。【结论】分析认为D01井新近系较太古界高出热流主要为高孔渗岩溶白云岩层中地下水侧向热对流作用以及牛东断裂地下水垂向热对流作用共同所致。研究结果对前人提出的地下水运移聚热模式及导热断裂聚热模式提供了数据支撑,对雄安新区深部地热资源成因机制和太古界地温场研究具有重要意义。     

雄安新区地热水的化学场特征及影响因素分析

【研究目的】雄安新区地热水化学场特征及其影响因素对了解区域地热资源聚敛机制具有重要意义。【研究方法】在区内5个主要构造单元（容城凸起、牛驼镇凸起、霸县凹陷、保定凹陷和高阳低凸起）开展地热水水化学采样和测试分析工作。【研究结果】研究区内主要分布有砂岩热储和岩溶热储,水化学类型以Cl-Na型和Cl·HCO₃-Na为主。从浅入深,地热水TDS值呈增大趋势。自西向东,地热水TDS含量表现为增大的趋势,指示着地下水流向。受断裂带导水作用影响,部分深部雾迷山组与馆陶组地热水发生混合现象。雾迷山组岩溶热储地热水的变质系数和脱硫系数低,热储封闭性较好,处于相对还原状态,而馆陶组和明化镇组砂岩热储地热水封闭性相对较差。【结论】区内地下水化学场主要受水岩相互作用程度、断裂、储层封闭性等因素影响。研究成果对于认识雄安新区地热资源、科学合理开发利用地热能,推进北方地区冬季清洁取暖具有重要意义。     

基于卡尔曼滤波的GPS高动态载波跟踪环路设计

针对高动态环境会使接收机接收信号载频上产生很大的多普勒频移及其变化率,普通的GPS载波跟踪环无法保证可靠的跟踪等问题,通过综合分析传统的二阶叉积自动频率控制环(CPAFC)辅助三阶锁相环(PLL)的高动态载波跟踪环路,以及卡尔曼滤波器在动态跟踪中的优势与劣势,该文设计了一种基于卡尔曼滤波的二阶CPAFC辅助三阶PLL的GPS高动态载波跟踪环路。通过仿真分析证明,新的环路能更好地适应动态性,整体跟踪性能更好;并且在信噪比较低的情况下,环路优势更明显。